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68 médias trouvés pour 'Nsf'

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Training for mothers, 1930s (b/w photo)

Training for mothers, 1930s (b/w photo)

SZT2983644

Rally of the National Socialist Women's League (NS-Frauenschaft) in the Luitpoldhalle at the 1937 Reich Party Congress (b/w photo)

Rally of the National Socialist Women's League (NS-Frauenschaft) in the Luitpoldhalle at the 1937 Reich Party Congress (b/w photo)

Scherl

SZT6310132

Children's group of the National Socialist Women's League, 1943 (b/w photo)

Children's group of the National Socialist Women's League, 1943 (b/w photo)

SZT3668056

SENATORS' ARVEDSON SKATES BY MOCK NSF CHEQUES DURING GAME IN EDMONTON, 2003-01-11 (photo)

SENATORS' ARVEDSON SKATES BY MOCK NSF CHEQUES DURING GAME IN EDMONTON, 2003-01-11 (photo)

Dan Riedlhuber

REU8284519

Mother's course at the National Socialist Women's League, 1943 (b/w photo)

Mother's course at the National Socialist Women's League, 1943 (b/w photo)

SZT3668050

Members of the National Socialist Women's League making straw sandals, 1941 (b/w photo)

Members of the National Socialist Women's League making straw sandals, 1941 (b/w photo)

SZT3668052

Meeting of the National Socialist Women's League in the Sports Palace in Berlin, 1934 (b/w photo)

Meeting of the National Socialist Women's League in the Sports Palace in Berlin, 1934 (b/w photo)

SZT3668065

Gertrud Scholtz-Klink at the Nuremberg Rally, 1935 (b/w photo)

Gertrud Scholtz-Klink at the Nuremberg Rally, 1935 (b/w photo)

SZT3668049

Members of the National Socialist Women's League making Christmas decoration, 1941 (b/w photo)

Members of the National Socialist Women's League making Christmas decoration, 1941 (b/w photo)

SZT3668055

Sophie Fikentscher and the National Socialist Women's League, Berlin 1939 (b/w photo)

Sophie Fikentscher and the National Socialist Women's League, Berlin 1939 (b/w photo)

SZT3668042

Children's group of the National Socialist Women's League, 1943 (b/w photo)

Children's group of the National Socialist Women's League, 1943 (b/w photo)

SZT3668046

Workshop of the National Socialist Women's League, 1943 (b/w photo)

Workshop of the National Socialist Women's League, 1943 (b/w photo)

SZT3668043

Children's group of the National Socialist Women's League, 1943 (b/w photo)

Children's group of the National Socialist Women's League, 1943 (b/w photo)

SZT3668057

Children's group of the National Socialist Women's League, 1943 (b/w photo)

Children's group of the National Socialist Women's League, 1943 (b/w photo)

SZT3668058

Members of the National Socialist Women's League help evacuated families, 1943 (b/w photo)

Members of the National Socialist Women's League help evacuated families, 1943 (b/w photo)

SZT3668044

Members of the National Socialist Women's League making toys, 1943 (b/w photo)

Members of the National Socialist Women's League making toys, 1943 (b/w photo)

SZT3668059

War workshop of the National Socialist Women's League, 1944 (b/w photo)

War workshop of the National Socialist Women's League, 1944 (b/w photo)

SZT3668060

Sewing workshop of the National Socialist Women's League, 1943 (b/w photo)

Sewing workshop of the National Socialist Women's League, 1943 (b/w photo)

SZT3668047

Harvest helpers of the National Socialist Women's League, 1940 (b/w photo)

Harvest helpers of the National Socialist Women's League, 1940 (b/w photo)

SZT3668062

War Auxiliary Service of the National Socialist Women's League in Belgium, 1940 (b/w photo)

War Auxiliary Service of the National Socialist Women's League in Belgium, 1940 (b/w photo)

SZT3668054

National Socialist Women's League helping refugees in France, 1940 (b/w photo)

National Socialist Women's League helping refugees in France, 1940 (b/w photo)

SZT3668040

Members of the National Socialist Women's League with Otto Mehlan in the gardening school in Berlin-Wilmersdorf, 1942 (b/w photo)

Members of the National Socialist Women's League with Otto Mehlan in the gardening school in Berlin-Wilmersdorf, 1942 (b/w photo)

SZT3668053

Romanian Natl. Salvation Front supporters puch an anti-Front protestor from a tank at the NSF Headquarters, Bucharest, 1990-01-28 (photo)

Romanian Natl. Salvation Front supporters puch an anti-Front protestor from a tank at the NSF Headquarters, Bucharest, 1990-01-28 (photo)

Popescu, Adrian

REU11939091

Paul von Hase, Fanni Luukkonen and Else Paul in Berlin, 1943 (b/w photo)

Paul von Hase, Fanni Luukkonen and Else Paul in Berlin, 1943 (b/w photo)

SZT3668051

Members of the National Socialist Women's League at the Nuremberg Rally, 1936 (b/w photo)

Members of the National Socialist Women's League at the Nuremberg Rally, 1936 (b/w photo)

SZT3668061

Sewing workshop of the National Socialist Women's League, 1943 (b/w photo)

Sewing workshop of the National Socialist Women's League, 1943 (b/w photo)

SZT3668048

NS speaker at an event of the Scherl publishing house, Berlin 1938 (b/w photo)

NS speaker at an event of the Scherl publishing house, Berlin 1938 (b/w photo)

SZT3668041

Protestors with banner saying National Salvation front = Romanian Communist Party have their way blocked by police and soldiers as they march to NSF HQ, Bucharest, 1990-01-24 (photo)

Protestors with banner saying National Salvation front = Romanian Communist Party have their way blocked by police and soldiers as they march to NSF HQ, Bucharest, 1990-01-24 (photo)

Popescu, Adrian

REU12002018

Air show of the NSFK in Hamburg-Fuhlsbuettel 1937

Air show of the NSFK in Hamburg-Fuhlsbuettel 1937

Scherl

SZT5179653

Thousands of Romanians supporting the Liberal PArty and supporters of the National Salvation Front have their way blocked by soldiers and tanks as they try to march onto the NSF headquaters, 1990-01-28 (photo)

Thousands of Romanians supporting the Liberal PArty and supporters of the National Salvation Front have their way blocked by soldiers and tanks as they try to march onto the NSF headquaters, 1990-01-28 (photo)

Popescu, Adrian

REU11939053

Bessarabia Germans in a transit camp in Belgrade, 1940 (b/w photo)

Bessarabia Germans in a transit camp in Belgrade, 1940 (b/w photo)

SZT2984421

Rudolf Hess giving medals to members of the National Socialist Woman's League, 1940 (b/w photo)

Rudolf Hess giving medals to members of the National Socialist Woman's League, 1940 (b/w photo)

SZT3024774

Having a meal during the resettlement of the Lithuania Germans, 1941 (b/w photo)

Having a meal during the resettlement of the Lithuania Germans, 1941 (b/w photo)

SZT3023646

Grossflugtag (Day of flying) in Berlin-Tempelhof, 1930s

Grossflugtag (Day of flying) in Berlin-Tempelhof, 1930s

Knorr + Hirth

SZT5179652

The exhibition "Einsatz der Frau in der Nation" before the 1937 Nuremberg Party Congress (b/w photo)

The exhibition "Einsatz der Frau in der Nation" before the 1937 Nuremberg Party Congress (b/w photo)

Scherl

SZT6310172

NS-Frauenschaft (National Socialist Women's League) helping with evacuation, 1943

NS-Frauenschaft (National Socialist Women's League) helping with evacuation, 1943

SZT5179664

III Reich - Gauführer School Sachsenburg Castle 1933 (photo)

III Reich - Gauführer School Sachsenburg Castle 1933 (photo)

SZT9226054

II. WK, Nazi Women's Society, 1930/40s (photo)

II. WK, Nazi Women's Society, 1930/40s (photo)

SZT9229263

SENATORS' REDDEN SKATES BY SIGN HELD BY EDMONTON FAN DURING GAME
AGAINST OILERS, 2003-01-12 (photo) — SENATORS' REDDEN SKATES BY SIGN HELD BY EDMONTON FAN DURING GAME AGAINST OILERS, 2003-01-12 (photo)

SENATORS' REDDEN SKATES BY SIGN HELD BY EDMONTON FAN DURING GAME AGAINST OILERS, 2003-01-12 (photo)

Dan Riedlhuber

REU8464275

PRESIDENT CLINTON WIPES HIS FACE AT NAF CONFERENCE IN ANAHEIM, 1999-07-09 (photo)

PRESIDENT CLINTON WIPES HIS FACE AT NAF CONFERENCE IN ANAHEIM, 1999-07-09 (photo)

Sam Mircovich

REU8467066

Third Reich - Anschluss of Austria 1938 (photo)

Third Reich - Anschluss of Austria 1938 (photo)

SZT9052722

Third Reich - Anschluss of Austria 1938 (photo)

Third Reich - Anschluss of Austria 1938 (photo)

SZT9052773

WW2 - NS Women's Union 1941 (photo)

WW2 - NS Women's Union 1941 (photo)

SZT9052396

III Reich, Anschluss of Austria, 1938 (photo)

III Reich, Anschluss of Austria, 1938 (photo)

SZT9229210

WW2 - NS Women's Union 1940 (photo)

WW2 - NS Women's Union 1940 (photo)

SZT9052774

II. WK - NS Women's Union, 1944 (photo)

II. WK - NS Women's Union, 1944 (photo)

SZT9234693

II. WK, war economy, 1944 (photo)

II. WK, war economy, 1944 (photo)

SZT9239131

II. WK, NS Women's Union 1944 (photo)

II. WK, NS Women's Union 1944 (photo)

SZT11748257

II. WK, NS Women's Union 1944 (photo)

II. WK, NS Women's Union 1944 (photo)

SZT11748574

WW2 - NS Women's Union 1939 (photo)

WW2 - NS Women's Union 1939 (photo)

SZT9052721

II. WK, NS Women's Union, 1942 (photo)

II. WK, NS Women's Union, 1942 (photo)

SZT9229003

II. WK, NS Women's Union around 1943 (photo)

II. WK, NS Women's Union around 1943 (photo)

SZT11747998

Eagle Nebula (IC 4703) and star cluster M16 in the Snake - This wide - field image of the Eagle Nebula was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Located in the constellation of Serpens, the Serpent, the Eagle Nebula is a very luminous open cluster of stars surrounded by dust and gas. The three pillars at the center of the image, made famous in an image by the Hubble Space Telescope, are being sculpted by the intense radiation from the hot stars in the cluster. This image was created by combining emission - line images in Hydrogen - alpha (green), Oxygen [O III] (blue) and Sulfur [S II] (red)

Eagle Nebula (IC 4703) and star cluster M16 in the Snake - This wide - field image of the Eagle Nebula was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Located in the constellation of Serpens, the Serpent, the Eagle Nebula is a very luminous open cluster of stars surrounded by dust and gas. The three pillars at the center of the image, made famous in an image by the Hubble Space Telescope, are being sculpted by the intense radiation from the hot stars in the cluster. This image was created by combining emission - line images in Hydrogen - alpha (green), Oxygen [O III] (blue) and Sulfur [S II] (red)

PIX4619986

Nebula of the cone NGC 2264 in the Unicorn - Nebulae in Monoceros - The nebula of the Cone below, is a region about 2600 years - light from the Earth. The bright star in the high center is S Monocerotis, a star of magnitude 4.7. Nests in these gas clouds, the Christmas tree, a cluster of young stars whose shape evokes a Christmas tree. This wide - field image of the Christmas Tree Cluster was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Also known as NGC2264, it is an open cluster of stars embedded in a diffuse nebula. It is located in the constellation of Monoceros, the Unicorn. The image also contains two famous nebula. At the bottom center of the image is the Cone Nebula, and to the upper left is the Fox Fur Nebula. The bright star just above the center of the image is known as S Mon. The gentle arcs in orange and blue near the center of the image are Herbig Haro objects, jets of gas from protostars embedded in the nebula. This image was created by combining emission - line images in Hydrogen - alpha (red - orange), Oxygen [O III] (light blue) and Sulfur [S II] (blue - violet) — Nebula of the cone NGC 2264 in the Unicorn - Nebulae in Monoceros - The nebula of the Cone below, is a region about 2600 years - light from the Earth. The bright star in the high center is S Monocerotis, a star of magnitude 4.7. Nests in these gas clouds, the Christmas tree, a cluster of young stars whose shape evokes a Christmas tree. This wide - field image of the Christmas Tree Cluster was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Also known as NGC2264, it is an open cluster of stars embedded in a diffuse nebula. It is located in the constellation of Monoceros, the Unicorn. The image also contains two famous nebula. At the bottom center of the image is the Cone Nebula, and to the upper left is the Fox Fur Nebula. The bright star just above the center of the image is known as S Mon. The gentle arcs in orange and blue near the center of the image are Herbig Haro objects, jets of gas from protostars embedded in the ne

Nebula of the cone NGC 2264 in the Unicorn - Nebulae in Monoceros - The nebula of the Cone below, is a region about 2600 years - light from the Earth. The bright star in the high center is S Monocerotis, a star of magnitude 4.7. Nests in these gas clouds, the Christmas tree, a cluster of young stars whose shape evokes a Christmas tree. This wide - field image of the Christmas Tree Cluster was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Also known as NGC2264, it is an open cluster of stars embedded in a diffuse nebula. It is located in the constellation of Monoceros, the Unicorn. The image also contains two famous nebula. At the bottom center of the image is the Cone Nebula, and to the upper left is the Fox Fur Nebula. The bright star just above the center of the image is known as S Mon. The gentle arcs in orange and blue near the center of the image are Herbig Haro objects, jets of gas from protostars embedded in the ne

PIX4618652

Solar stain and granulation. Image obtained by the solar telescope of Sacramento Peak-USA - False color picture of a sunspot taken with the National Solar Observatory's Vacuum Tower Telescope at the Sacramento Peak Observatory.: Surface du Soleil - Sunspot

Solar stain and granulation. Image obtained by the solar telescope of Sacramento Peak-USA - False color picture of a sunspot taken with the National Solar Observatory's Vacuum Tower Telescope at the Sacramento Peak Observatory.: Surface du Soleil - Sunspot

PIX4626765

Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years

Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years

PIX4620086

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright star near the center of the image is Eta Carinae, which is one of the most massive and luminous stars known. This picture is a composite of several exposures made with the Curtis - Schmidt telescope at the Cerro Tololo Interamerican Observatory — Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

PIX4618865

Remains of the Crab Supernova (M1) in the Taurus - This image of the well - known Crab Nebula was taken using Ektachrome film at the prime focus of the Kitt Peak 4 - meter telescope on October 1st 1973. This is unusual because most astronomical pictures are coloured by combining three different exposures taken through red, green and blue filters. In this relatively short exposure, the pulsar is clearly visible (slightly below and to the right of the central star, which is actually a projected foreground object). North is up with east to the left

Remains of the Crab Supernova (M1) in the Taurus - This image of the well - known Crab Nebula was taken using Ektachrome film at the prime focus of the Kitt Peak 4 - meter telescope on October 1st 1973. This is unusual because most astronomical pictures are coloured by combining three different exposures taken through red, green and blue filters. In this relatively short exposure, the pulsar is clearly visible (slightly below and to the right of the central star, which is actually a projected foreground object). North is up with east to the left

PIX4583005

Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m telescope on Kitt Peak with the Mosaic camera, and is presented here in false color (hydrogen alpha, OIII oxygen, and SII sulfur red respectively, green and blue, using five ten - minute exposures each). The Rosette is a prominent star formation region, glowing due to ultraviolet light from the young, hot, blue stars whose winds also cleared the central hole. It is enormously large on the sky, covering more than six times the area of the full moon — Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

PIX4618453

Swan Lace - detail ngc 6960 - This image of the Veil Nebula was taken with the Mosaic camera on the WIYN 0.9 - meter telescope at the National Science Foundation's Kitt Peak National Observatory near Tucson, AZ. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light - years from Earth in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova

Swan Lace - detail ngc 6960 - This image of the Veil Nebula was taken with the Mosaic camera on the WIYN 0.9 - meter telescope at the National Science Foundation's Kitt Peak National Observatory near Tucson, AZ. The Veil Nebula (NGC 6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light - years from Earth in the direction of the constellation Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova

PIX4582687

Solar Oscillations - Oscillations of the Sun - Computer image showing solar acoustic oscillation patterns. By measuring these frequencies, astronomers obtain information about the internal structure of a star. This color picture is a computer representation of one of nearly ten million modes of sound wave oscillations of the Sun, showing receding regions in red tones and approaching regions in blue. By measuring the frequencies of many such modes and using theoretical models, solar astronomers can infer much about the internal structure and dynamics of the Sun. This technique is called helioseismology, because of its similarities to terrestrial seismology, and is at the heart of the NOAO program called the Global Oscillation Network Group (GONG). GONG operates an international network of instrument stations that provide continuous measurements of such oscillations, by always having a station in daylight at all times

Solar Oscillations - Oscillations of the Sun - Computer image showing solar acoustic oscillation patterns. By measuring these frequencies, astronomers obtain information about the internal structure of a star. This color picture is a computer representation of one of nearly ten million modes of sound wave oscillations of the Sun, showing receding regions in red tones and approaching regions in blue. By measuring the frequencies of many such modes and using theoretical models, solar astronomers can infer much about the internal structure and dynamics of the Sun. This technique is called helioseismology, because of its similarities to terrestrial seismology, and is at the heart of the NOAO program called the Global Oscillation Network Group (GONG). GONG operates an international network of instrument stations that provide continuous measurements of such oscillations, by always having a station in daylight at all times

PIX4627270

Remains of the Crab Supernova (M1) in the Taurus and Crab Pulsar - This picture shows a time sequence for the pulsar in the Crab nebula, shown in context against an image, also taken with the Kitt Peak 4 - meter Mayall telescope. Both the nebula and its central pulsar were created by a supernova explosion in the year 1054 A.D. The enlarged region is a mosaic of 33 time slices, ordered from top to bottom and from left to right. Each slice represents approximately one millisecond in the period of the pulsar. The brighter, primary pulse is visible in the first column: the weaker, broader inter - pulse can be seen in the second column. These data were taken with the Kitt Peak Photon Counting Array (KPCA) at the Kitt Peak 4 - meter Mayall telescope during the night of 20 October 1989, using a standard B - band optical filter, and represent a phased accumulation of almost two hours of observation. The observed period at the telescope was 33.36702 milliseconds. Due to poor weather and a long exposure seeing of more than 3.5 arc seconds, each slice was sharpened by computer image processing before making the mosaic. The KPCA was capable of millisecond time resolution for both imaging and spectroscopy, predominantly at blue wavelengths — Remains of the Crab Supernova (M1) in the Taurus and Crab Pulsar - This picture shows a time sequence for the pulsar in the Crab nebula, shown in context against an image, also taken with the Kitt Peak 4 - meter Mayall telescope. Both the nebula and its central pulsar were created by a supernova explosion in the year 1054 A.D. The enlarged region is a mosaic of 33 time slices, ordered from top to bottom and from left to right. Each slice represents approximately one millisecond in the period of the pulsar. The brighter, primary pulse is visible in the first column: the weaker, broader inter - pulse can be seen in the second column. These data were taken with the Kitt Peak Photon Counting Array (KPCA) at the Kitt Peak 4 - meter Mayall telescope during the night of 20 October 1989, using a standard B - band optical filter, and represent a phased accumulation of almost two hours of observation. The observed period at the telescope was 33.36702 milliseconds. Due to poor weather and a long

Remains of the Crab Supernova (M1) in the Taurus and Crab Pulsar - This picture shows a time sequence for the pulsar in the Crab nebula, shown in context against an image, also taken with the Kitt Peak 4 - meter Mayall telescope. Both the nebula and its central pulsar were created by a supernova explosion in the year 1054 A.D. The enlarged region is a mosaic of 33 time slices, ordered from top to bottom and from left to right. Each slice represents approximately one millisecond in the period of the pulsar. The brighter, primary pulse is visible in the first column: the weaker, broader inter - pulse can be seen in the second column. These data were taken with the Kitt Peak Photon Counting Array (KPCA) at the Kitt Peak 4 - meter Mayall telescope during the night of 20 October 1989, using a standard B - band optical filter, and represent a phased accumulation of almost two hours of observation. The observed period at the telescope was 33.36702 milliseconds. Due to poor weather and a long

PIX4583092

Spiral galaxy M33 in triangle - Optical compsite - radio - M33, NGC598 Triangle galaxy about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Visible are stars and star-forming regions (red). The radio image shows the cold hydrogen (blue - purple). Images obtained with the 90 cm telescope of Kitt Peak (visible) and with the radiotelescopes of the VLA and WRST (radio

Spiral galaxy M33 in triangle - Optical compsite - radio - M33, NGC598 Triangle galaxy about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Visible are stars and star-forming regions (red). The radio image shows the cold hydrogen (blue - purple). Images obtained with the 90 cm telescope of Kitt Peak (visible) and with the radiotelescopes of the VLA and WRST (radio

PIX4609273

Galaxy Centaurus A (NGC 5128) in visible and infrared - Galaxy Centaurus A in visible and infrared - The galaxy NGC 5128 is about 13 million years away - light from Earth. This an elliptical galaxy that cannibalized a small spiral galaxy. The infrared image, on the right, reveals the complex structure of the central dust strip. Images obtained on the left by Cerro Tololo's 4m telescope and on the right by the Spitzer space telescope. Centaurus A (NGC 5128) is the nearest active galaxy to Earth. Located 13 million light - years away in the southern constellation Centaurus, 'Cen A' appears to be the result of a merger - collision between a large elliptical galaxy (which has a black hole at its center) and a smaller spiral galaxy that veered too close to the larger one, resulting in the cannabalization of the small galaxy. The visible image (left) from the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile is dominated by a bright halo of light caused by the stars in the galaxy. Many of these stars are hidden by the dense band of dust that blocks our view of their light. Infrared light is not so readily obscured by dust as visible light, so the infrared image (right) from instruments on the NASA - JPL Spitzer Space Telescope reveals the complex structure of the dust lane, and the stars and gas embedded within it — Galaxy Centaurus A (NGC 5128) in visible and infrared - Galaxy Centaurus A in visible and infrared - The galaxy NGC 5128 is about 13 million years away - light from Earth. This an elliptical galaxy that cannibalized a small spiral galaxy. The infrared image, on the right, reveals the complex structure of the central dust strip. Images obtained on the left by Cerro Tololo's 4m telescope and on the right by the Spitzer space telescope. Centaurus A (NGC 5128) is the nearest active galaxy to Earth. Located 13 million light - years away in the southern constellation Centaurus, 'Cen A' appears to be the result of a merger - collision between a large elliptical galaxy (which has a black hole at its center) and a smaller spiral galaxy that veered too close to the larger one, resulting in the cannabalization of the small galaxy. The visible image (left) from the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile is dominated by a brigh

Galaxy Centaurus A (NGC 5128) in visible and infrared - Galaxy Centaurus A in visible and infrared - The galaxy NGC 5128 is about 13 million years away - light from Earth. This an elliptical galaxy that cannibalized a small spiral galaxy. The infrared image, on the right, reveals the complex structure of the central dust strip. Images obtained on the left by Cerro Tololo's 4m telescope and on the right by the Spitzer space telescope. Centaurus A (NGC 5128) is the nearest active galaxy to Earth. Located 13 million light - years away in the southern constellation Centaurus, 'Cen A' appears to be the result of a merger - collision between a large elliptical galaxy (which has a black hole at its center) and a smaller spiral galaxy that veered too close to the larger one, resulting in the cannabalization of the small galaxy. The visible image (left) from the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile is dominated by a brigh

PIX4612203

Irregular Galaxy M82 in the Great Bear - The irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind (visible in red). Image obtained by the 3.5m WIYN telescope at Kitt Peak and completed by data obtained by the Hubble space telescope. This image is a color - coded picture of the archetypal starburst galaxy M82. It shows the horizontal stellar disk of the galaxy, which harbors its active star formation, and a perpendicular supergalactic wind of ionized gas powered by the energy released in the starburst. To make this image, data from the WIYN 3.5 - meter telescope on Kitt Peak were combined with data from the WFPC2 camera on the Hubble Space Telescope. Purple represents emission in ionized hydrogen (H - alpha) and ionized nitrogen, and the green is ionized sulfur in the WIYN data — Irregular Galaxy M82 in the Great Bear - The irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind (visible in red). Image obtained by the 3.5m WIYN telescope at Kitt Peak and completed by data obtained by the Hubble space telescope. This image is a color - coded picture of the archetypal starburst galaxy M82. It shows the horizontal stellar disk of the galaxy, which harbors its active star formation, and a perpendicular supergalactic wind of ionized gas powered by the energy released in the starburst. To make this image, data from the WIYN 3.5 - meter telescope on Kitt Peak were combined with data from the WFPC2 camera on the Hubble Space Telescope. Purple represents e

Irregular Galaxy M82 in the Great Bear - The irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind (visible in red). Image obtained by the 3.5m WIYN telescope at Kitt Peak and completed by data obtained by the Hubble space telescope. This image is a color - coded picture of the archetypal starburst galaxy M82. It shows the horizontal stellar disk of the galaxy, which harbors its active star formation, and a perpendicular supergalactic wind of ionized gas powered by the energy released in the starburst. To make this image, data from the WIYN 3.5 - meter telescope on Kitt Peak were combined with data from the WFPC2 camera on the Hubble Space Telescope. Purple represents e

PIX4610403

Supernova 1987A and Tarantula Nebula - Supernova 1987A in the Large Magellanic Cloud appears as a very bright object near the center of this color photograph. The photograph was taken at Noao's Cerro - Tololo Inter - American Observatory, on March 2nd 1987, using the Curtis Schmidt telescope

Supernova 1987A and Tarantula Nebula - Supernova 1987A in the Large Magellanic Cloud appears as a very bright object near the center of this color photograph. The photograph was taken at Noao's Cerro - Tololo Inter - American Observatory, on March 2nd 1987, using the Curtis Schmidt telescope

PIX4582306

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. Their stars are more than 12 billion years old, and, in most cases, formed all at once when the universe was just a toddler. Omega Centauri is unusual in that its stars are of different ages and possess varying levels of metals, or elements heavier than boron. Astronomers say this points to a different origin for Omega Centauri than other globular clusters: they think it might be the core of a dwarf galaxy that was ripped apart and absorbed by our Milky Way long ago. In this picture of Omega Centauri, the red - and yellow - colored dots represent the stars revealed by Spitzer. These are the more evolved, larger, dustier stars, called red giants. The stars colored blue are less evolved, like our own sun, and were captured by both Spitzer's infrared eyes and in visible light by the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile. Some of the red spots in the picture are distant ga — Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

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Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and exploded. Recent observations of the remnant of SN 1006 reveal the liberation of elements such as iron that were previously locked up inside the star. Because no material falls back into a neutron star or black hole after this type of supernova explosion, the liberation of this star's contents is complete. This is a composite image of the SN 1006 supernova remnant, which is located about 7000 light years from Earth. Shown here are X - ray data from Nasa's Chandra X - ray Observatory (blue), optical data from the University of Michigan's 0.9 meter Curtis Schmidt telescope at the NSF's Cerro Tololo Inter - American Observatory (CTIO; yellow) and the Digitized Sky Survey (orange and light blue), plus radio data from the NRAO's Very Large Array and Green Bank Telescope (VLA/GB/GBV T ; red) — Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

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