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Images of 'Asymmetric' found, 80

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Sketch of a swimsuit, 1965 (marker on paper)

Sketch of a swimsuit, 1965 (marker on paper)

Blass, Bill (1922-2002)

IMA374314

Modern "Decorator" bowl, c.1959 (silverplate & plastic)

Modern "Decorator" bowl, c.1959 (silverplate & plastic)

Gorham Manufacturing Company

XDM1071839

The First German Gymnastics Festival in Coburg, 1860

The First German Gymnastics Festival in Coburg, 1860

SZT3020237

England / UK: Sir Isaac Newton's asymmetric colour wheel correlating colours with musical notes and planetary symbols. London, 1704

England / UK: Sir Isaac Newton's asymmetric colour wheel correlating colours with musical notes and planetary symbols. London, 1704

PFH2561692

BELGIAN SABRINA BURLINETTO PERFORMS ON THE ASYMMETRIC BARS AT THE WORLD
ARTISTIC GYMNASTIC ..., 2001-10-29 (photo) — BELGIAN SABRINA BURLINETTO PERFORMS ON THE ASYMMETRIC BARS AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-10-29 (photo)

BELGIAN SABRINA BURLINETTO PERFORMS ON THE ASYMMETRIC BARS AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-10-29 (photo)

Thierry Roge

REU8532218

Vase with asymmetric handles, 1935, lustred polychrome black and silvery ceramic, Deruta manufacture, Italy, 20th century

Vase with asymmetric handles, 1935, lustred polychrome black and silvery ceramic, Deruta manufacture, Italy, 20th century

Italian School, (20th century)

DGA928066

Atoms, Elements & Molecules, Models Models illustrating Van't Hoff's theory of the asymmetric carbon atom, c 1874

Atoms, Elements & Molecules, Models Models illustrating Van't Hoff's theory of the asymmetric carbon atom, c 1874

UIS5083219

A model for Carolina Herrera wears a shell silk jersey over a asymmetric sleeveless flounce hem dres.., 1999 (photo)

A model for Carolina Herrera wears a shell silk jersey over a asymmetric sleeveless flounce hem dres.., 1999 (photo)

Jeff Christensen

REU7478313

COJOCAR OF ROMANIA PERFORMS ON ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT
WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo) — COJOCAR OF ROMANIA PERFORMS ON ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo)

COJOCAR OF ROMANIA PERFORMS ON ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo)

Yves Herman

REU8417234

COURTNEY KUPEST OF UNITED STATES PERFORMS IN WOMEN'S ASYMMETRIC BARS AT
36TH WORLD GYMNASTICS ..., 2002-11-23 (photo) — COURTNEY KUPEST OF UNITED STATES PERFORMS IN WOMEN'S ASYMMETRIC BARS AT 36TH WORLD GYMNASTICS ..., 2002-11-23 (photo)

COURTNEY KUPEST OF UNITED STATES PERFORMS IN WOMEN'S ASYMMETRIC BARS AT 36TH WORLD GYMNASTICS ..., 2002-11-23 (photo)

Laszlo Balogh

REU7767354

HEENAN OF THE U.S. PEFORMS AT ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT
THE WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo) — HEENAN OF THE U.S. PEFORMS AT ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo)

HEENAN OF THE U.S. PEFORMS AT ASYMMETRIC BARS IN WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-10-31 (photo)

Yves Herman

REU7905152

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

Aalto, Alvar (1898-1976)

Mark Edward Smith

MES3502953

COUNTREY KUPEST OF UNITED STATES PERFORMS IN THE WOMEN'S APPARATUS ASYMMETRIC BARS AT 36TH WORLD GYMNASTICS CHAMPIONSHIPS IN DEBRECEN, 2002 (photo)

COUNTREY KUPEST OF UNITED STATES PERFORMS IN THE WOMEN'S APPARATUS ASYMMETRIC BARS AT 36TH WORLD GYMNASTICS CHAMPIONSHIPS IN DEBRECEN, 2002 (photo)

Laszlo Balogh

REU7488727

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

Aalto, Alvar (1898-1976)

Mark Edward Smith

MES3502988

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202521

The Green Citadel of Magdeburg (Hundertwasser Haus), detail of North East tower
Magdeburg, Saxony-Anhalt, Germany (photo) — The Green Citadel of Magdeburg (Hundertwasser Haus), detail of North East tower Magdeburg, Saxony-Anhalt, Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), detail of North East tower Magdeburg, Saxony-Anhalt, Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202517

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202527

View of the Bell Tower, Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

View of the Bell Tower, Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

Aalto, Alvar (1898-1976)

Mark Edward Smith

MES3502984

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

View of the exterior of Church of Santa Maria Assunta by Alvar Aalto, Riola di Vergato, Emilia Romagna, Italy (photo)

Aalto, Alvar (1898-1976)

Mark Edward Smith

MES3502959

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202515

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202518

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202525

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202522

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202530

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202526

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202514

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202520

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202523

The Citicorp Building, designed by Hugh Stubbins & Associates in 1978 (photo)

The Citicorp Building, designed by Hugh Stubbins & Associates in 1978 (photo)

Singer, Barbara

SNG137805

Sketch of an evening dress, 1975 (marker on paper)

Sketch of an evening dress, 1975 (marker on paper)

Blass, Bill (1922-2002)

IMA374319

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202519

Wrinkle ridges are a very common landform on Mars, Mercury, Venus, and the Moon. These ridges are linear to arcuate asymmetric topographic highs commonly found on smooth plains.

Wrinkle ridges are a very common landform on Mars, Mercury, Venus, and the Moon. These ridges are linear to arcuate asymmetric topographic highs commonly found on smooth plains.

UIG866514

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202528

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202524

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202516

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

The Green Citadel of Magdeburg (Hundertwasser Haus), Germany (photo)

Hundertwasser, Friedensreich (1928-2000)

Chinch Gryniewicz

POV1202529

Beaded cocktail gown, Coco Chanel, c.1927 (photo)

Beaded cocktail gown, Coco Chanel, c.1927 (photo)

CH622612

My Model, young woman posing, holding sword, engraving by Ernesto Mancastroppa from painting by Andrea Petroni (1863-1943), from L'Illustrazione Italiana, year 18, no 29, July 19, 1891

My Model, young woman posing, holding sword, engraving by Ernesto Mancastroppa from painting by Andrea Petroni (1863-1943), from L'Illustrazione Italiana, year 18, no 29, July 19, 1891

Mancastroppa, Ernesto (1857-1909)

DGA5654282

Felix-Nussbaum-Museum, Osnabrueck, Germany (photo)

Felix-Nussbaum-Museum, Osnabrueck, Germany (photo)

ARD2549438

Zakim Bridge and steps along the Charles River, Boston, USA (photo)

Zakim Bridge and steps along the Charles River, Boston, USA (photo)

WTL487274

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This picture of the Meathook Galaxy (NGC 2442) was taken by the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla, Chile. This view includes the whole galaxy and the surrounding sky, and clearly shows the asymmetric spiral arms. The longer of the two arms has intense star formation, which is visible here as a pink glow: this is due to the radiation of young stars ionising the gas they form from. The asymmetric shape and star formation are both thought to be caused by tidal disruptions from a near - miss with another galaxy at some point in its history

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This picture of the Meathook Galaxy (NGC 2442) was taken by the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla, Chile. This view includes the whole galaxy and the surrounding sky, and clearly shows the asymmetric spiral arms. The longer of the two arms has intense star formation, which is visible here as a pink glow: this is due to the radiation of young stars ionising the gas they form from. The asymmetric shape and star formation are both thought to be caused by tidal disruptions from a near - miss with another galaxy at some point in its history

PIX4610133

Miranda Cicognani at the Olympic Games

Miranda Cicognani at the Olympic Games

Sergio del Grande

MEP2347930

COURTNEY KUPEST OF UNITED STATES TALKS TO HER TEAM MATE ASHLEY POSTELL
AFTER SHE WON WOMEN'S ..., 2002-11-23 (photo) — COURTNEY KUPEST OF UNITED STATES TALKS TO HER TEAM MATE ASHLEY POSTELL AFTER SHE WON WOMEN'S ..., 2002-11-23 (photo)

COURTNEY KUPEST OF UNITED STATES TALKS TO HER TEAM MATE ASHLEY POSTELL AFTER SHE WON WOMEN'S ..., 2002-11-23 (photo)

Laszlo Balogh

REU7730403

Spiral galaxy NGC 1961 in Giraffe - NGC 1961 spiral galaxy in Camelopardalis - Spiral galaxy NGC 1961 (Arp 184) in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1961 (Arp 184) is a problematic galaxy. Its highly disturbed and asymmetric spiral arms would normally indicate an interaction or merger with another galaxy. However, no culprit is found to be the source of NGC 1961's angst. Given the apparent size and brightness of this galaxy - it must be one of the largest galaxies in our “” local”” universe. The shape of the galaxy may be due to its interaction with the gas in the cluster. Most of this galaxy is still producing young and massive stars that live short lives and die violent deaths as supernovae

Spiral galaxy NGC 1961 in Giraffe - NGC 1961 spiral galaxy in Camelopardalis - Spiral galaxy NGC 1961 (Arp 184) in the constellation Giraffe. Image made with a telescope of 61 cm. NGC 1961 (Arp 184) is a problematic galaxy. Its highly disturbed and asymmetric spiral arms would normally indicate an interaction or merger with another galaxy. However, no culprit is found to be the source of NGC 1961's angst. Given the apparent size and brightness of this galaxy - it must be one of the largest galaxies in our “” local”” universe. The shape of the galaxy may be due to its interaction with the gas in the cluster. Most of this galaxy is still producing young and massive stars that live short lives and die violent deaths as supernovae

Adam Block

PIX4609981

Venetian Nobleman

Venetian Nobleman

EPL6872182

Galaxy clusters 1ES 0657 - 55 in the Carene - Gravitational lens in galaxy cluster 1ES 0657 - 55 - False color image of the distant galaxy cluster 1ES 0657 - 55 in the southern constellation of Carene obtained by the VLT. A gravitational mirage is visible in the form of a green arc at the top right of the image; it is the image of an even farther away galaxy curved and amplified by the gravity of this cluster. An Arc at z = 3.23 in galaxy cluster 1ES 0657 - 55. The galaxy cluster 1ES 0657 - 55 is located in the southern constellation Carina (The Keel), south of the Milky Way band. Its redshift has been measured as z = 0.29. It is a source of strong and very hot X - ray emission and has an asymmetric galaxy distribution, indicating a large mass and recent formation

Galaxy clusters 1ES 0657 - 55 in the Carene - Gravitational lens in galaxy cluster 1ES 0657 - 55 - False color image of the distant galaxy cluster 1ES 0657 - 55 in the southern constellation of Carene obtained by the VLT. A gravitational mirage is visible in the form of a green arc at the top right of the image; it is the image of an even farther away galaxy curved and amplified by the gravity of this cluster. An Arc at z = 3.23 in galaxy cluster 1ES 0657 - 55. The galaxy cluster 1ES 0657 - 55 is located in the southern constellation Carina (The Keel), south of the Milky Way band. Its redshift has been measured as z = 0.29. It is a source of strong and very hot X - ray emission and has an asymmetric galaxy distribution, indicating a large mass and recent formation

PIX4565630

MODEL WEARS FASHIONS FROM DONNA KARAN FALL 2001 COLLECTION, 2001-02-16 (photo)

MODEL WEARS FASHIONS FROM DONNA KARAN FALL 2001 COLLECTION, 2001-02-16 (photo)

Mike Segar

REU8263634

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M 66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. The galaxy forms, together with its neighbours M65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The asymmetric appearance is most likely due to gravitational interaction with its neighbours

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M 66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. The galaxy forms, together with its neighbours M65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The asymmetric appearance is most likely due to gravitational interaction with its neighbours

Jim Misti

PIX4610833

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. The galaxy forms, together with its neighbours M65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The asymmetric appearance is most likely due to gravitational interaction with its neighbours

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. The galaxy forms, together with its neighbours M65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The asymmetric appearance is most likely due to gravitational interaction with its neighbours

Adam Block

PIX4610847

SCHIAPARELLI GOWN 1950S

SCHIAPARELLI GOWN 1950S

Barnaby's Studios Ltd, (20th century)

EPL6859247

MODEL WEARS A SILK DRESS AT THE CAROLINA HERRERA FASHION SHOW, 1999-09-13 (photo)

MODEL WEARS A SILK DRESS AT THE CAROLINA HERRERA FASHION SHOW, 1999-09-13 (photo)

Jeff Christensen

REU8484379

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

SZT11749079

FILE PICTURE OF A ROMANIAN AIRBUS A310 WHICH CRASHED IN 1995, 2000-12-18 (photo)

FILE PICTURE OF A ROMANIAN AIRBUS A310 WHICH CRASHED IN 1995, 2000-12-18 (photo)

Radu Sigheti

REU7880919

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble Space Telescope and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble Space Telescope and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

PIX4610093

Women's fashion, 1942 (b/w photo)

Women's fashion, 1942 (b/w photo)

SZT2986945

MODEL WEARS FASHIONS FROM HELMUT LANG FALL 2001 COLLECTION, 2001-02-15 (photo)

MODEL WEARS FASHIONS FROM HELMUT LANG FALL 2001 COLLECTION, 2001-02-15 (photo)

Mike Segar

REU8218894

Holger Schilp of German online service, Comcity 0nline Services, tests a computer in front of screen.., 1998 (photo)

Holger Schilp of German online service, Comcity 0nline Services, tests a computer in front of screen.., 1998 (photo)

Peter Mueller

REU7471849

KHORKINA OF RUSSIA PERFORMS DURING WORLD ARTISTIC GYMNASTIC
CHAMPIONSHIPS, 2001-11-02 (photo) — KHORKINA OF RUSSIA PERFORMS DURING WORLD ARTISTIC GYMNASTIC CHAMPIONSHIPS, 2001-11-02 (photo)

KHORKINA OF RUSSIA PERFORMS DURING WORLD ARTISTIC GYMNASTIC CHAMPIONSHIPS, 2001-11-02 (photo)

Yves Herman

REU8595187

A WORKER TEST A COMPUTER ON THE CEBIT HOME FAIR IN HANOVER, 1998-08-25 (photo)

A WORKER TEST A COMPUTER ON THE CEBIT HOME FAIR IN HANOVER, 1998-08-25 (photo)

Peter Mueller

REU8226142

A Viennese porcelain-mounted giltwood cabinet-on-stand, c. 1880

A Viennese porcelain-mounted giltwood cabinet-on-stand, c. 1880

Austrian School, (19th century)

CH11991851

OLYMPIC CHAMPION SVETLANA KHORKINA OF RUSSIA STEPS IN MAGNESIA AS SHE
WARMS UP FOR THE BEAM FINAL, 2002-11-24 (photo) — OLYMPIC CHAMPION SVETLANA KHORKINA OF RUSSIA STEPS IN MAGNESIA AS SHE WARMS UP FOR THE BEAM FINAL, 2002-11-24 (photo)

OLYMPIC CHAMPION SVETLANA KHORKINA OF RUSSIA STEPS IN MAGNESIA AS SHE WARMS UP FOR THE BEAM FINAL, 2002-11-24 (photo)

Laszlo Balogh

REU7821535

NOBEL ECONOMICS PRIZEWINNER AKERLOF SPEAKS AT PRESS CONFERENCE, 2001-10-10 (photo)

NOBEL ECONOMICS PRIZEWINNER AKERLOF SPEAKS AT PRESS CONFERENCE, 2001-10-10 (photo)

Lou Dematteis

REU8375062

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained at the VLT in December 2001. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. Many regions of warm hydrogen gas are seen throughout the disc of this galaxy. The latter regions are being ionised by radiation from clusters of newborn stars. Very active star - formation is most likely also occurring in the nuclear regions of NGC 3627.The galaxy forms, together with its neighbours M 65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The asymmetric appearance is most likely due to gravitational interaction with its neighbours. This image was taken on 16 - 18 December 2001 with the VLT — Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained at the VLT in December 2001. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. Many regions of warm hydrogen gas are seen throughout the disc of this galaxy. The latter regions are being ionised by radiation from clusters of newborn stars. Very active star - formation is most likely also occurring in the nuclear regions of NGC 3627.The galaxy forms, together with its neighbours M 65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The as

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained at the VLT in December 2001. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. Many regions of warm hydrogen gas are seen throughout the disc of this galaxy. The latter regions are being ionised by radiation from clusters of newborn stars. Very active star - formation is most likely also occurring in the nuclear regions of NGC 3627.The galaxy forms, together with its neighbours M 65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The as

PIX4610814

Rachitic children, 1919 (b/w photo)

Rachitic children, 1919 (b/w photo)

SZT3011123

NOBEL PRIZE WINNER IN ECONOMICS AKERLOF SMILES AT PRESS CONFERENCE, 2001-10-10 (photo)

NOBEL PRIZE WINNER IN ECONOMICS AKERLOF SMILES AT PRESS CONFERENCE, 2001-10-10 (photo)

Lou Dematteis

REU8361708

Fashions at the Royal Ascot Races, Berkshire, 16 June 1936

Fashions at the Royal Ascot Races, Berkshire, 16 June 1936

UIS5067794

NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT
THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo) — NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo)

NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo)

Yves Herman

REU8595214

NOBEL ECONOMICS PRIZE WINNER AKERLOF SPEAKS AT PRESS CONFERENCE, 2001-10-10 (photo)

NOBEL ECONOMICS PRIZE WINNER AKERLOF SPEAKS AT PRESS CONFERENCE, 2001-10-10 (photo)

Lou Dematteis

REU8496180

NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT
THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo) — NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo)

NATALIA ZIGANSHIVA OF RUSSIA PERFORMS DURING THE WOMEN'S TEAM FINAL AT THE WORLD ARTISTIC GYMNASTIC ..., 2001-11-02 (photo)

Yves Herman

REU8585650

Fine Damascus poison cup, c.12th century (brass)

Fine Damascus poison cup, c.12th century (brass)

Syrian School, (12th century)

CH3082221

JOSEPH STIGLITZ AWARDED NOBLE PRIZE FOR ECONOMICS, 2001-10-10 (photo)

JOSEPH STIGLITZ AWARDED NOBLE PRIZE FOR ECONOMICS, 2001-10-10 (photo)

Brad Rickerby

REU8458618

Sperm Whale and Fin Whale, 1850 (lithography)

Sperm Whale and Fin Whale, 1850 (lithography)

Tenhaeff, J. W. (19th century)

PRX11961656

Album Page: House of Worth, Costume, 1910-11 (b/w photo)

Album Page: House of Worth, Costume, 1910-11 (b/w photo)

French Photographer, (20th century)

FMB3513133

Album Page: House of Worth, Jacket, 1908-10 (b/w photo)

Album Page: House of Worth, Jacket, 1908-10 (b/w photo)

French Photographer, (20th century)

FMB3514175

Album Page: House of Worth, Ball Gown, 1909-10 (b/w photo)

Album Page: House of Worth, Ball Gown, 1909-10 (b/w photo)

French Photographer, (20th century)

FMB3513154

Medallion carpet, probably Persian Kurdistan, late 17th or early 18th century (wool & cotton)

Medallion carpet, probably Persian Kurdistan, late 17th or early 18th century (wool & cotton)

CH3041429

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past observers. Many supernovae - - the explosions of hot, blue, short - lived stars at least eight times the mass of the Sun - - have gone off in the core of the Whale Galaxy. The stellar pyrotechnics have bathed the galaxy in hot gas, visible to X - ray telescopes like ESA's XMM - Newton. Comparing the optical and near - infrared observations from Hubble with other telescopes sensitive to different wavelengths of light helps astronomers gather the full story behind celestial phenomena. From such work, the triggers of the starburst in the Whale Galaxy and others can be elucidated. The gravitational “” feeding”” on intergalactic material, as well as clumping caused by the gravitational interactions with its galactic neighbours, creates the areas of greater density where stars start to coalesce. Just as blue whales, the biggest creatures on Earth, can gorge themselves on comparatively tiny bits of plankton, so the Whale Galaxy has become filled with the gas and dust that p — Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

PIX4611784

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astronomers believe that Messier 66's once orderly shape has most likely been distorted by the gravitational pull of its two neighbours. Hubble has imaged Messier 66's striking dust lanes and bright star clusters along the spiral arms in fine detail with the Advanced Camera for Surveys. Star clusters - - pictured in the blue and pinkish regions of the image - - are key tools for astronomers since they are used as indicators of how the parent galaxies assembled over time. Messier 66 boasts a remarkable record of supernovae explosions. The spiral galaxy has hosted three supernovae since 1989, the latest one occurring in 2009. A supernova is a stellar explosion that may momentarily outshine its entire host galaxy. It then fades away over a period lasting several weeks or months. During its very short life the supernova radiates as much energy as the Sun would radiate over a period of about 10 billion years — Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

PIX4610836

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

SZT11749206

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

II. WK, Luftwaffe, Blohm and Voss 1942 (photo)

SZT11749080

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