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781485 Search Results for Photography

Issue Apostrophes - Portrait of Pascal Quignard October 28, 2002
Issue Apostrophes - Portrait of Pascal Quignard October 28, 2002

SOB4886864: Issue Apostrophes - Portrait of Pascal Quignard October 28, 2002 / Bridgeman Images

ID: SOB4886864

Issue Apostrophes - Portrait of Pascal Quignard October 28, 2002

Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Spitzer were found in four dark cores, or stellar “” incubators,””” where stars are born. Astronomers using data from the Institute of Radioastronomy millimeter telescope in Spain had previously identified these cores but thought they were not quite ripe for stars. Spitzer's highly sensitive infrared eyes were able to penetrate all four cores to reveal rapidly growing embryos. Astronomers can actually count the individual embryos tucked inside the cores by looking closely at the Spitzer image taken by its infrared array camera (top right). This instrument has the highest spatial resolution of Spitzer's imaging cameras. The Spitzer image from the multiband imaging photometer (bottom right), on the other hand, specializes in detecting cooler materials. Its view highlights the relatively cool core material falling onto the Trifidi's growing embryos. The middle panel is a combination of Spitzer data from both of these instruments. The embryos are thought to have been triggered by a massiv
Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Spitzer were found in four dark cores, or stellar “” incubators,””” where stars are born. Astronomers using data from the Institute of Radioastronomy millimeter telescope in Spain had previously identified these cores but thought they were not quite ripe for stars. Spitzer's highly sensitive infrared eyes were able to penetrate all four cores to reveal rapidly growing embryos. Astronomers can actually count the individual embryos tucked inside the cores by looking closely at the Spitzer image taken by its infrared array camera (top right). This instrument has the highest spatial resolution of Spitzer's imaging cameras. The Spitzer image from the multiband imaging photometer (bottom right), on the other hand, specializes in detecting cooler materials. Its view highlights the relatively cool core material falling onto the Trifidi's growing embryos. The middle panel is a combination of Spitzer data from both of these instruments. The embryos are thought to have been triggered by a massiv

PIX4619569: Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Spitzer were found in four dark cores, or stellar “” incubators,””” where stars are born. Astronomers using data from the Institute of Radioastronomy millimeter telescope in Spain had previously identified these cores but thought they were not quite ripe for stars. Spitzer's highly sensitive infrared eyes were able to penetrate all four cores to reveal rapidly growing embryos. Astronomers can actually count the individual embryos tucked inside the cores by looking closely at the Spitzer image taken by its infrared array camera (top right). This instrument has the highest spatial resolution of Spitzer's imaging cameras. The Spitzer image from the multiband imaging photometer (bottom right), on the other hand, specializes in detecting cooler materials. Its view highlights the relatively cool core material falling onto the Trifidi's growing embryos. The middle panel is a combination of Spitzer data from both of these instruments. The embryos are thought to have been triggered by a massiv / Bridgeman Images

ID: PIX4619569

Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Sp

Planetary Nebula M 27 (NGC 6853) in the Little Fox - M27 The Dumbbell Nebula Astro - Physic's 130 EDT f/8 Composite of two exposures, 12 minutes and 60 minutes hypered Fuji Super G 800 8:36 and 8:55 pm October 7, 1994 Mt. Pinos, C
Planetary Nebula M 27 (NGC 6853) in the Little Fox - M27 The Dumbbell Nebula Astro - Physic's 130 EDT f/8 Composite of two exposures, 12 minutes and 60 minutes hypered Fuji Super G 800 8:36 and 8:55 pm October 7, 1994 Mt. Pinos, C

PIX4623426: Planetary Nebula M 27 (NGC 6853) in the Little Fox - M27 The Dumbbell Nebula Astro - Physic's 130 EDT f/8 Composite of two exposures, 12 minutes and 60 minutes hypered Fuji Super G 800 8:36 and 8:55 pm October 7, 1994 Mt. Pinos, C / Bridgeman Images

ID: PIX4623426

Planetary Nebula M 27 (NGC 6853) in the Little Fox - M27 The Dumbbell Nebula Astro - Physic's 130 EDT f/8 Composite of two exposures, 12 minutes and 60 minutes hypered Fuji Super G 800 8:36 and 8:55 pm October 7, 1994 Mt. Pinos, C

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its overall appearance. Objects like CRL2688 are rare because they are in an evolutionary phase which lasts for a very short time (~ 1,000 to 2,000 years). However, they may hold the key to our understanding of how red giant stars transform themselves into planetary nebulae. For the first time, we can see a 10,000 year - old history of mass - ejection in a red giant star in such exquisite detail. The arcs in CRL2688 represent dense shells of matter within a smooth cloud, and show that the rate of mass ejection from the central star has varied on time scales of ~ 100 to 500 years throughout its mass - loss history. With Hubble we have detected matter in this nebula to a radius of 0.6 light - years - - much further out than has been possible before, giving a better estimate of the amount of matter in the nebula. Other unexpected results seen in this image are the very sharply defined edges of the beams and fine spoke - like features which suggest that, contrary to previous models, the searchli
Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its overall appearance. Objects like CRL2688 are rare because they are in an evolutionary phase which lasts for a very short time (~ 1,000 to 2,000 years). However, they may hold the key to our understanding of how red giant stars transform themselves into planetary nebulae. For the first time, we can see a 10,000 year - old history of mass - ejection in a red giant star in such exquisite detail. The arcs in CRL2688 represent dense shells of matter within a smooth cloud, and show that the rate of mass ejection from the central star has varied on time scales of ~ 100 to 500 years throughout its mass - loss history. With Hubble we have detected matter in this nebula to a radius of 0.6 light - years - - much further out than has been possible before, giving a better estimate of the amount of matter in the nebula. Other unexpected results seen in this image are the very sharply defined edges of the beams and fine spoke - like features which suggest that, contrary to previous models, the searchli

PIX4623752: Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its overall appearance. Objects like CRL2688 are rare because they are in an evolutionary phase which lasts for a very short time (~ 1,000 to 2,000 years). However, they may hold the key to our understanding of how red giant stars transform themselves into planetary nebulae. For the first time, we can see a 10,000 year - old history of mass - ejection in a red giant star in such exquisite detail. The arcs in CRL2688 represent dense shells of matter within a smooth cloud, and show that the rate of mass ejection from the central star has varied on time scales of ~ 100 to 500 years throughout its mass - loss history. With Hubble we have detected matter in this nebula to a radius of 0.6 light - years - - much further out than has been possible before, giving a better estimate of the amount of matter in the nebula. Other unexpected results seen in this image are the very sharply defined edges of the beams and fine spoke - like features which suggest that, contrary to previous models, the searchli / Bridgeman Images

ID: PIX4623752

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

22/04/2009 Rome, concert du musicien et chanteur americain Ben Harper sur la Piazza del popolo.
22/04/2009 Rome, concert du musicien et chanteur americain Ben Harper sur la Piazza del popolo.

AGF5492120: 22/04/2009 Rome, concert du musicien et chanteur americain Ben Harper sur la Piazza del popolo. / Bridgeman Images

ID: AGF5492120

22/04/2009 Rome, concert du musicien et chanteur americain Ben Harper sur la Piazza del popolo.

Tatiana Grindenko, Russian violinist, & Rosa Fain, Ukrainian violinist, Hanover, 2000 (photo)
Tatiana Grindenko, Russian violinist, & Rosa Fain, Ukrainian violinist, Hanover, 2000 (photo)

PUT5455531: Tatiana Grindenko, Russian violinist, & Rosa Fain, Ukrainian violinist, Hanover, 2000 (photo) / Bridgeman Images

ID: PUT5455531

Tatiana Grindenko, Russian violinist, & Rosa Fain, Ukrainian violinist, Hanover, 2000 (photo)

Alphons Diepenbrock; Dutch; composer;1911
Alphons Diepenbrock; Dutch; composer;1911

PUT5455547: Alphons Diepenbrock; Dutch; composer;1911 / Bridgeman Images

ID: PUT5455547

Alphons Diepenbrock; Dutch; composer;1911

JEAN MIOTTE 1994
JEAN MIOTTE 1994

MLO5674181: JEAN MIOTTE 1994 / Bridgeman Images

ID: MLO5674181

JEAN MIOTTE 1994

laurence Cochet 1994
laurence Cochet 1994

MLO5674194: laurence Cochet 1994 / Bridgeman Images

ID: MLO5674194

laurence Cochet 1994

manifestation en 1968 Champs Elysees
manifestation en 1968 Champs Elysees

MLO5674198: manifestation en 1968 Champs Elysees / Bridgeman Images

ID: MLO5674198

manifestation en 1968 Champs Elysees

manifestation en 1968 Champs Elysees
manifestation en 1968 Champs Elysees

MLO5674199: manifestation en 1968 Champs Elysees / Bridgeman Images

ID: MLO5674199

manifestation en 1968 Champs Elysees

Pierrette Fleutiaux
Pierrette Fleutiaux

MLO5674236: Pierrette Fleutiaux / Bridgeman Images

ID: MLO5674236

Pierrette Fleutiaux

Pierrette Fleutiaux
Pierrette Fleutiaux

MLO5674238: Pierrette Fleutiaux / Bridgeman Images

ID: MLO5674238

Pierrette Fleutiaux

TAHAR BEN JELLOUN 1989
TAHAR BEN JELLOUN 1989

MLO5674243: TAHAR BEN JELLOUN 1989 / Bridgeman Images

ID: MLO5674243

TAHAR BEN JELLOUN 1989

thierry saussez
thierry saussez

MLO5674245: thierry saussez / Bridgeman Images

ID: MLO5674245

thierry saussez

Tomi Ungerer en 1989 a strasbourg
Tomi Ungerer en 1989 a strasbourg

MLO5674250: Tomi Ungerer en 1989 a strasbourg / Bridgeman Images

ID: MLO5674250

Tomi Ungerer en 1989 a strasbourg

YVES COURRIERE 1986
YVES COURRIERE 1986

MLO5674252: YVES COURRIERE 1986 / Bridgeman Images

ID: MLO5674252

YVES COURRIERE 1986

Philippe Muray
Philippe Muray

MLO5673809: Philippe Muray / Bridgeman Images

ID: MLO5673809

Philippe Muray

FRANCOISE XENAKIS 1986
FRANCOISE XENAKIS 1986

MLO5674124: FRANCOISE XENAKIS 1986 / Bridgeman Images

ID: MLO5674124

FRANCOISE XENAKIS 1986

FRANCOISE XENAKIS 1986
FRANCOISE XENAKIS 1986

MLO5674125: FRANCOISE XENAKIS 1986 / Bridgeman Images

ID: MLO5674125

FRANCOISE XENAKIS 1986

JEAN DES CARS 1986
JEAN DES CARS 1986

MLO5674127: JEAN DES CARS 1986 / Bridgeman Images

ID: MLO5674127

JEAN DES CARS 1986

BEATRICE DIDIER 1994
BEATRICE DIDIER 1994

MLO5674137: BEATRICE DIDIER 1994 / Bridgeman Images

ID: MLO5674137

BEATRICE DIDIER 1994

Belloc (denis ) 1994
Belloc (denis ) 1994

MLO5674140: Belloc (denis ) 1994 / Bridgeman Images

ID: MLO5674140

Belloc (denis ) 1994

CABU 1988
CABU 1988

MLO5674146: CABU 1988 / Bridgeman Images

ID: MLO5674146

CABU 1988

Dalil BOUBAKEUR 1994
Dalil BOUBAKEUR 1994

MLO5674150: Dalil BOUBAKEUR 1994 / Bridgeman Images

ID: MLO5674150

Dalil BOUBAKEUR 1994

Gerard Oury 1988
Gerard Oury 1988

MLO5674158: Gerard Oury 1988 / Bridgeman Images

ID: MLO5674158

Gerard Oury 1988

Ceremonial Textile (Nambu With Tigma Design) (photo)
Ceremonial Textile (Nambu With Tigma Design) (photo)

IMA1556876: Ceremonial Textile (Nambu With Tigma Design) (photo), Tibetan School (19th century) / Bridgeman Images

ID: IMA1556876

Ceremonial Textile (Nambu With Tigma Design) (photo)

Tibetan School (19th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558494: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558494

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558495: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558495

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558498: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558498

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558503: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558503

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558524: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558524

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558528: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558528

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558536: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558536

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558541: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558541

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)

Shirt Panel (Mola) (photo)
Shirt Panel (Mola) (photo)

IMA1558544: Shirt Panel (Mola) (photo), Kuna Indian Culture (20th century) / Bridgeman Images

ID: IMA1558544

Shirt Panel (Mola) (photo)

Kuna Indian Culture (20th century)


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