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Immagini di 'Doppiamente' trovate, 35

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Bystander - Making assurance doubly sure

Bystander - Making assurance doubly sure

Cleaver, Ralph (1870-1938)

EPL7004683

A new art-if-ice - doubly hazardous (engraving)

A new art-if-ice - doubly hazardous (engraving)

Cruikshank, George (1792-1878)

LLJ585162

Illustration for The Deserted Village by Oliver Goldsmith (colour litho)

Illustration for The Deserted Village by Oliver Goldsmith (colour litho)

Hankey, William Lee (1869-1952)

LLM5992174

Leaf edges margins crenate, dentate, entire, doubly serrate, lobate, serrate, sinuate, spiny, undulate

Leaf edges margins crenate, dentate, entire, doubly serrate, lobate, serrate, sinuate, spiny, undulate

DGA1259895

UTAH JAZZ STOCKTON IS DOUBLE TEAMED BY SONICS PAYTON AND GRANT, 2000-04-29 (photo)

UTAH JAZZ STOCKTON IS DOUBLE TEAMED BY SONICS PAYTON AND GRANT, 2000-04-29 (photo)

Reuters Photographer

REU7905208

And kissed her thoughtless babes with many a tear, and clapsed them close, in sorrow doubly dear (colour litho)

And kissed her thoughtless babes with many a tear, and clapsed them close, in sorrow doubly dear (colour litho)

Hankey, William Lee (1869-1952)

IL955983

The Transit Instrument. It Consists of an Achromatic Telescope, to which is Firmly Fixed a Doubly Conical and Horizontal Axis, at Right Angles to the Optical Axis of the Telescope

The Transit Instrument. It Consists of an Achromatic Telescope, to which is Firmly Fixed a Doubly Conical and Horizontal Axis, at Right Angles to the Optical Axis of the Telescope

LZT1003073

Mill Street, Warwick (photo)

Mill Street, Warwick (photo)

English Photographer, (20th century)

LLM727543

DENMARK'S THOMAS BJORN LEAVES THE 16TH HOLE WHICH HE DOUBLE BOGEYED
DURING THE LAST DAY OF THE BRITISH ..., 2003-07-20 (photo) — DENMARK'S THOMAS BJORN LEAVES THE 16TH HOLE WHICH HE DOUBLE BOGEYED DURING THE LAST DAY OF THE BRITISH ..., 2003-07-20 (photo)

DENMARK'S THOMAS BJORN LEAVES THE 16TH HOLE WHICH HE DOUBLE BOGEYED DURING THE LAST DAY OF THE BRITISH ..., 2003-07-20 (photo)

Darren Staples

REU7657181

RAPTORS CARTER DOUBLE TEAMED BY TIMBERWOLVES SMITH AND SZCZERBIAK, 2000-02-26 (photo)

RAPTORS CARTER DOUBLE TEAMED BY TIMBERWOLVES SMITH AND SZCZERBIAK, 2000-02-26 (photo)

Peter Jones

REU7847764

RAPTORS CARTER FIGHTS FOR REBOUND WITH GRIZZLIES RAHIM AND HARRINGTON, 2000-03-05 (photo)

RAPTORS CARTER FIGHTS FOR REBOUND WITH GRIZZLIES RAHIM AND HARRINGTON, 2000-03-05 (photo)

Lyle Stafford

REU7839431

WARRIORS CAFFEY TRAPPED IN CELTICS DOUBLE TEAM, 2000-03-16 (photo)

WARRIORS CAFFEY TRAPPED IN CELTICS DOUBLE TEAM, 2000-03-16 (photo)

Brian Snyder

REU7741543

Satirical cartoon, The Effects of Hope!

Satirical cartoon, The Effects of Hope!

Cruikshank, Isaac (1756-1811)

EPL6908445

JAZZ STOCKTON DOUBLE TEAMED BY SONICS PAYTON AND BAKER, 2000-04-29 (photo)

JAZZ STOCKTON DOUBLE TEAMED BY SONICS PAYTON AND BAKER, 2000-04-29 (photo)

Reuters Photographer

REU7948379

LOS ANGELES LAKERS SHAQUILLE ONEAL DOUBLE TEAMED, 2000-06-10 (photo)

LOS ANGELES LAKERS SHAQUILLE ONEAL DOUBLE TEAMED, 2000-06-10 (photo)

Mike Blake

REU7971502

WOODS HITS FROM FAIRWAY DURING FINAL ROUND OF THE TOUR CHAMPIONSHIP IN
ATLANTA, 2002-11-03 (photo) — WOODS HITS FROM FAIRWAY DURING FINAL ROUND OF THE TOUR CHAMPIONSHIP IN ATLANTA, 2002-11-03 (photo)

WOODS HITS FROM FAIRWAY DURING FINAL ROUND OF THE TOUR CHAMPIONSHIP IN ATLANTA, 2002-11-03 (photo)

Tami Chappell

REU8068172

Mata Hari

Mata Hari

EPL6790896

FORMER ALL BLACK WILSON ANNOUNCES RETIREMENT IN CHRISTCHURCH, NEW
ZEALAND, 2002-05-19 (photo) — FORMER ALL BLACK WILSON ANNOUNCES RETIREMENT IN CHRISTCHURCH, NEW ZEALAND, 2002-05-19 (photo)

FORMER ALL BLACK WILSON ANNOUNCES RETIREMENT IN CHRISTCHURCH, NEW ZEALAND, 2002-05-19 (photo)

Simon Baker

REU7796488

Christmas greetings postcard with dance-related poem

Christmas greetings postcard with dance-related poem

EPL6953658

II. WK - Paratrooper, 1943 (photo)

II. WK - Paratrooper, 1943 (photo)

SZT9233835

Advert for Burberrys tielocken trench coats 1916

Advert for Burberrys tielocken trench coats 1916

EPL6946435

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Sverre A. Børretzen

NTB8968002

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows how, as the blue component is concentrated in very dense clumps which act to protect the neutral oxygen from the intense ultraviolet radiation which has ionized the other gas components. The Dumbbell nebula is about 850 light - years away from Earth and about 1.5 light - years in diameter — Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

PIX4623419

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen — Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

PIX4620193

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen — Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

PIX4620159

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Sverre A. Børretzen

NTB8967408

Advert for Burberry tielocken trench coats 1916

Advert for Burberry tielocken trench coats 1916

EPL6895532

II. WK, Afrikafeldzug, Africa Corps 1942 (photo)

II. WK, Afrikafeldzug, Africa Corps 1942 (photo)

SZT11748736

II. WK - Eastern Front - MG gunners, 1942 (photo)

II. WK - Eastern Front - MG gunners, 1942 (photo)

SZT9234573

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated the 800th anniversary for the creation of the Archbishop's chair …, 1953 (photo)

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated the 800th anniversary for the creation of the Archbishop's chair …, 1953 (photo)

Sverre A. Børretzen

NTB8617554

Stiklestad 19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Stiklestad 19530815. The Protestant and Catholic Church in Norway celebrated …, 1953 (photo)

Sverre A. Børretzen

NTB8967640

Remnants of the Crab Supernova (M1) in the Taurus - This is a mosaic image, one of the largest ever taken by Nasa's Hubble Space Telescope of the Crab Nebula, a six - light - year - wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans. The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra - dense core of the exploded star. The Crab Nebula derived its name from its appearance in a drawing made by Irish astronomer Lord Rosse in 1844, using a 36 - inch telescope. When viewed by Hubble, as well as by large ground - based telescopes such as the European Southern Observatory's Very Large Telescope, the Crab Nebula takes on a more detailed appearance that yields clues into the spectacular demise of a star, 6,500 light - years away. The newly composed image was assembled from 24 individual Wide Field and Planetary Camera 2 exposures taken in October 1999, January 2000, and December 2000. The colors in the image indicate the different elements that were expelled during the explosion. Blue in the filaments in the outer part of the nebula represents neutral oxygen, green is singly - ionized sulfur, and red indicates doubly - ionized oxygen — Remnants of the Crab Supernova (M1) in the Taurus - This is a mosaic image, one of the largest ever taken by Nasa's Hubble Space Telescope of the Crab Nebula, a six - light - year - wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans. The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra - dense core of the exploded star. The Crab Nebula derived its name from its appearance in a dra

Remnants of the Crab Supernova (M1) in the Taurus - This is a mosaic image, one of the largest ever taken by Nasa's Hubble Space Telescope of the Crab Nebula, a six - light - year - wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans. The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra - dense core of the exploded star. The Crab Nebula derived its name from its appearance in a dra

PIX4583010

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated the 800th …, 1953 (photo)

Trondheim19530815. The Protestant and Catholic Church in Norway celebrated the 800th …, 1953 (photo)

Sverre A. Børretzen

NTB8945868

Detail of the Eagle Nebula (M16) dans le serpent/HST - This eerie, dark structure, resembling an imaginary sea serpent's head, is a column of cool molecular hydrogen gas (two atoms of hydrogen in each molecule) and dust that is an incubator for new stars. The stars are embedded inside finger - like protrusions extending from the top of the nebula. Each “” fingertip”” is somewhat larger than our own solar system. The pillar is slowly eroding away by the ultraviolet light from nearby hot stars, a process called “” photoevaporation””. As it does, small globules of especially dense gas buried within the cloud is uncovered. These globules have been dubbed “” Eggs”” - - an acronym for “” Evaporating Gaseous Globules””. The shadows of the Eggs protect gas behind them, resulting in the finger - like structures at the top of the cloud. Forming inside at least some of the Eggs are embryonic stars - - stars that abruptly stop growing when the Eggs are uncovered and they are separated from the larger reservoir of gas from which they were drawing mass. Eventually the stars emerge, as the Eggs themselves succumb to photoevaporation. The stellar EGGS are found, appropriately enough, in the “” Eagle Nebula”” (also called M16 - - the 16th object in Charles Messier's 18th century catalog of “” fuzzy”” permanent objects in the sky), a nearby star - forming region 6,500 light - years away in the constellation Serpens. The picture was taken on April 1, 1995 with the Hubble Space Telescope Wide Field and Planetary Camera 2. The color image is constructed from three separate images taken in the light of emission from different types of atoms. Red shows emission from singly - ionized sulfur atoms. Green shows emission from hydrogen. Blue shows light emitted by doubly - ionized oxygen atoms — Detail of the Eagle Nebula (M16) dans le serpent/HST - This eerie, dark structure, resembling an imaginary sea serpent's head, is a column of cool molecular hydrogen gas (two atoms of hydrogen in each molecule) and dust that is an incubator for new stars. The stars are embedded inside finger - like protrusions extending from the top of the nebula. Each “” fingertip”” is somewhat larger than our own solar system. The pillar is slowly eroding away by the ultraviolet light from nearby hot stars, a process called “” photoevaporation””. As it does, small globules of especially dense gas buried within the cloud is uncovered. These globules have been dubbed “” Eggs”” - - an acronym for “” Evaporating Gaseous Globules””. The shadows of the Eggs protect gas behind them, resulting in the finger - like structures at the top of the cloud. Forming inside at least some of the Eggs are embryonic stars - - stars that abruptly stop growing when the Eggs are uncovered and they are separated from the lar

Detail of the Eagle Nebula (M16) dans le serpent/HST - This eerie, dark structure, resembling an imaginary sea serpent's head, is a column of cool molecular hydrogen gas (two atoms of hydrogen in each molecule) and dust that is an incubator for new stars. The stars are embedded inside finger - like protrusions extending from the top of the nebula. Each “” fingertip”” is somewhat larger than our own solar system. The pillar is slowly eroding away by the ultraviolet light from nearby hot stars, a process called “” photoevaporation””. As it does, small globules of especially dense gas buried within the cloud is uncovered. These globules have been dubbed “” Eggs”” - - an acronym for “” Evaporating Gaseous Globules””. The shadows of the Eggs protect gas behind them, resulting in the finger - like structures at the top of the cloud. Forming inside at least some of the Eggs are embryonic stars - - stars that abruptly stop growing when the Eggs are uncovered and they are separated from the lar

PIX4620033

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a symmetry axis dramatically different from that of the larger hourglass. The hot star which has been thought to eject and illuminate the nebula, and therefore expected to lie at its center of symmetry, is clearly off center. Hubble has also revealed other features in MyCN18 which are completely new and unexpected. For example, there is a pair of intersecting elliptical rings in the central region which appear to be the rims of a smaller hourglass. There are the intricate patterns of the etchings on the hourglass walls. The arc - like etchings could be the remnants of discrete shells ejected from the star when it was younger (e.g. as seen in the Egg Nebula), flow instabilities, or could result from the action of a narrow beam of matter impinging on the hourglass walls. An unseen companion star and accompanying gravitational effects may well be necessary in order to explain the structure of myCN18. Distance: 8,000 light - years (2,500 parsecs) Exposure Date (s): July 30, 199 — Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

PIX4623735

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