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Type # for projects,to access projects, > for users, and ? for help.

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Bilder zu 'Pulled' gefunden, 4,118

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Boy leaning on a Windowsill, holding a Birdcage

Boy leaning on a Windowsill, holding a Birdcage

Netscher, Caspar (1639-84) (attr. to)

USB1161590

Switzerland Eiger Salvage, 1961 (b/w photo)

Switzerland Eiger Salvage, 1961 (b/w photo)

Stringer (STR)

KES6244771

A dhow episode: the capture of a slaver off the east coast of Africa, and the matrimonial agency which settled the freed slaves in life, 1893 (engraving)

A dhow episode: the capture of a slaver off the east coast of Africa, and the matrimonial agency which settled the freed slaves in life, 1893 (engraving)

Nash, Joseph (1809-78) (after)

MMM7339572

Street Patrol, Belfast, Northern Ireland, 1976 (oil on board)

Street Patrol, Belfast, Northern Ireland, 1976 (oil on board)

Lillford, Ralph (b.1932)

NAM5925057

Switzerland Eiger Salvage, 1957 (b/w photo)

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6244767

Portrait Bust of an Aristocratic Man and Portrait Bust of an Aristocratic Woman, c.270-280 (marble)

Portrait Bust of an Aristocratic Man and Portrait Bust of an Aristocratic Woman, c.270-280 (marble)

Roman Imperial Period (27 BC-476 AD)

XCL499618

Switzerland Eiger Salvage, 1957 (b/w photo)

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6245081

Switzerland Eiger Salvage, 1957 (b/w photo)

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6245079

Switzerland Eiger Salvage, 1959 (b/w photo)

Switzerland Eiger Salvage, 1959 (b/w photo)

Stringer (STR)

KES6244769

Switzerland Eiger Salvage, 1957 (b/w photo)

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6244770

Switzerland Eiger Salvage, 1959 (b/w photo)

Switzerland Eiger Salvage, 1959 (b/w photo)

Stringer (STR)

KES6244782

The Siege of Troy

The Siege of Troy

Morone, Domenico (c.1442-p.1517) (attr. to)

USB1158665

A Woman by a Window, probably Mercy Glazebook

A Woman by a Window, probably Mercy Glazebook

English School, (19th century)

USB1157476

South-East Gale at Portencross Castle, 1886 (oil on canvas)

South-East Gale at Portencross Castle, 1886 (oil on canvas)

Brett, John (1831-1902)

MAA2956910

Switzerland Eiger Salvage, 1957 (b/w photo)

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6245124

Phaeton alarm'd, 1808 (etching)

Phaeton alarm'd, 1808 (etching)

Gillray, James (1757-1815)

MMM7340077

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

PIX4612937

Switzerland Eiger Salvage, 1959 (b/w photo)

Switzerland Eiger Salvage, 1959 (b/w photo)

Stringer (STR)

KES6263862

A Punch Party

Patch, Thomas (1720-82)

USB1162600

Jupiter seen from his satellite Ganymede - Illustration - Ridges, grooves, and craters on Ganymede - Artist's view of the surface of Ganymede, Jupiter's largest satellite. An impact crater about 15 km in diameter differs from the striated surface of the satellite. In the sky are represented Jupiter, the Europe satellite on the top right, and Io on the left of Jupiter. Jupiter's largest satellite Ganymede has a varying surface, some of which is characterized by rumpled bundles of ridges and grooves that run for hundreds of miles over a frozen surface of water - ice. They probably formed long ago when tectonic forces pulled apart Ganymede's upper crust; similar sets of faults occur in rift zones on Earth, as in eastern Africa. Subsequent meteoritic impacts have peppered - - and broken in places - - the continuity of the running formations. In this image an impact crater about 10 miles in diameter dominates a scene otherwise defined by a dozen long ridges. In the middle of the crater is a

Jupiter seen from his satellite Ganymede - Illustration - Ridges, grooves, and craters on Ganymede - Artist's view of the surface of Ganymede, Jupiter's largest satellite. An impact crater about 15 km in diameter differs from the striated surface of the satellite. In the sky are represented Jupiter, the Europe satellite on the top right, and Io on the left of Jupiter. Jupiter's largest satellite Ganymede has a varying surface, some of which is characterized by rumpled bundles of ridges and grooves that run for hundreds of miles over a frozen surface of water - ice. They probably formed long ago when tectonic forces pulled apart Ganymede's upper crust; similar sets of faults occur in rift zones on Earth, as in eastern Africa. Subsequent meteoritic impacts have peppered - - and broken in places - - the continuity of the running formations. In this image an impact crater about 10 miles in diameter dominates a scene otherwise defined by a dozen long ridges. In the middle of the crater is a

Walter B Myers

PIX4575196

Rail Road March for the Fourth of July. Dedicated to the Directors of the Baltimore and Ohio Rail Road, 1828 (lithograph on paper)

Rail Road March for the Fourth of July. Dedicated to the Directors of the Baltimore and Ohio Rail Road, 1828 (lithograph on paper)

Willig, George Jnr (1794-1874)

IGM8836221

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Colliding spiral galaxies NGC 2207 and IC 2163 - Colliding galaxies NGC 2207 and IC 2163 - The galaxies NGC 2207 (left) and IC 2163 (right) form a pair of colliding galaxies approximately 114 million light years away. Currently IC 2163 is moving away from NGC 2207, but it is likely that within several billion years these two galaxies will eventually merge into a single massive galaxy. Image obtained by the Hubble Space Telescope in 1998. The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the Hubble Heritage image), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light - years towards the right - hand edge of the image. The calculations indicate that IC 2163 is swinging past NGC 2207 in a counterclockwise direction, having made its closest approach 40 million years ago. However, IC 2163 does not have sufficient ener

Colliding spiral galaxies NGC 2207 and IC 2163 - Colliding galaxies NGC 2207 and IC 2163 - The galaxies NGC 2207 (left) and IC 2163 (right) form a pair of colliding galaxies approximately 114 million light years away. Currently IC 2163 is moving away from NGC 2207, but it is likely that within several billion years these two galaxies will eventually merge into a single massive galaxy. Image obtained by the Hubble Space Telescope in 1998. The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the Hubble Heritage image), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light - years towards the right - hand edge of the image. The calculations indicate that IC 2163 is swinging past NGC 2207 in a counterclockwise direction, having made its closest approach 40 million years ago. However, IC 2163 does not have sufficient ener

PIX4610001

Action between the Dutch fleet and barbary pirates, c.1670 (oil painting)

Action between the Dutch fleet and barbary pirates, c.1670 (oil painting)

Verschuier, Lieve (1630-86)

MMM7337743

Farm Offensive - Producing Food For The War Effort

Farm Offensive - Producing Food For The War Effort

BOF6282629

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Sächsische Zeitung

IMO8758572

Group of Galaxies HCG 31 - Hickson Compact Group 31 - This group of interacting galaxies is located 166 million years of light from Earth in the constellation Eridan. Dwarf galaxies are merging causing intense star formation. This long fusion process will lead to the birth of a large elliptical galaxy. Image obtained by the Hubble Space Telescope on August 8, 2006. These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow. Such encounters between dwarf galaxies are normally seen billions of light - years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light - years away. In this image, taken by Nasa's Hubble Space Telescope, the

Group of Galaxies HCG 31 - Hickson Compact Group 31 - This group of interacting galaxies is located 166 million years of light from Earth in the constellation Eridan. Dwarf galaxies are merging causing intense star formation. This long fusion process will lead to the birth of a large elliptical galaxy. Image obtained by the Hubble Space Telescope on August 8, 2006. These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow. Such encounters between dwarf galaxies are normally seen billions of light - years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light - years away. In this image, taken by Nasa's Hubble Space Telescope, the

PIX4565530

Jupiter's Fusion Spots seen by the Hubble Space Telescope - Sequence of images of Jupiter's atmosphere obtained on May 15, June 28 and July 8, 2008 by the Hubble Space Telescope. The Great Red Spot of Jupiter is a gigantic permanent tempete measuring nearly 25,000 km in diameter. It's been observed for over 400 years. A second red spot half smaller, appeared in 2006; visible at the bottom of the image, we see it passing on this series below the Great red spot without being disturbed by the huge cyclone. A third red spot, visible at the extreme left on the first image appeared at the beginning of 2008. We see her heading towards the Great red spot to appear on the last clash deformed and almost colorless. It seems his destiny is to be totally swallowed by the Great Red Spot. The time series shows the passage of the “” Red Spot Jr.”” in a band of clouds below (south) of the Great Red Spot (GRS). “” Red Spot Jr.”” first appeared on Jupiter in early 2006 when a previously white storm turne

Jupiter's Fusion Spots seen by the Hubble Space Telescope - Sequence of images of Jupiter's atmosphere obtained on May 15, June 28 and July 8, 2008 by the Hubble Space Telescope. The Great Red Spot of Jupiter is a gigantic permanent tempete measuring nearly 25,000 km in diameter. It's been observed for over 400 years. A second red spot half smaller, appeared in 2006; visible at the bottom of the image, we see it passing on this series below the Great red spot without being disturbed by the huge cyclone. A third red spot, visible at the extreme left on the first image appeared at the beginning of 2008. We see her heading towards the Great red spot to appear on the last clash deformed and almost colorless. It seems his destiny is to be totally swallowed by the Great Red Spot. The time series shows the passage of the “” Red Spot Jr.”” in a band of clouds below (south) of the Great Red Spot (GRS). “” Red Spot Jr.”” first appeared on Jupiter in early 2006 when a previously white storm turne

PIX4574511

Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

PIX4565516

Prashand (10 years old) cleans debris of his fallen house with his sister Madhushika (12). Thotagamuwa village near Hikkaduwa, a popular tourist town in Southern Sri Lanka. He stated, I went to market to buy some fish and vegetables with my mother. We were walking on the side of the road (Galle Road from Colombo to Galle). Traffic was unusually heavy. I thought there must be an accident on the road ahead. Suddenly there was a big panic. Everyone was shouting and running. We also got frighten and started running back towards home, but it was too late. As soon as we turned, we got hit by a huge wave and sank. I was in the water for a long time and could not come out. I thought I was dying. I was still under water when my mother grabbed me and pulled me out. I dont know how long we were in the water. We kept rolling. It was like diving in the sea, only waves were far stronger. (photo)

Prashand (10 years old) cleans debris of his fallen house with his sister Madhushika (12). Thotagamuwa village near Hikkaduwa, a popular tourist town in Southern Sri Lanka. He stated, I went to market to buy some fish and vegetables with my mother. We were walking on the side of the road (Galle Road from Colombo to Galle). Traffic was unusually heavy. I thought there must be an accident on the road ahead. Suddenly there was a big panic. Everyone was shouting and running. We also got frighten and started running back towards home, but it was too late. As soon as we turned, we got hit by a huge wave and sank. I was in the water for a long time and could not come out. I thought I was dying. I was still under water when my mother grabbed me and pulled me out. I dont know how long we were in the water. We kept rolling. It was like diving in the sea, only waves were far stronger. (photo)

UIG795821

The King Carl XVI Gustaf with crown princess Victoria, 1980 (photo)

The King Carl XVI Gustaf with crown princess Victoria, 1980 (photo)

SJB7350073

2009 Military news report

2009 Military news report

BOF6287614

Victoria Cross group awarded to Field Marshal Lord Frederick Sleigh Roberts (metal)

Victoria Cross group awarded to Field Marshal Lord Frederick Sleigh Roberts (metal)

British School, (19th century)

NAM5926824

Victoria Cross group awarded to Field Marshal Lord Frederick Sleigh Roberts (metal)

Victoria Cross group awarded to Field Marshal Lord Frederick Sleigh Roberts (metal)

British School, (19th century)

NAM5926823

Lord John Hervey, 2nd Baron Hervey of Ickworth, PC, MP (1696-1743) holding his Purse of Office as Lord Privy Seal

Lord John Hervey, 2nd Baron Hervey of Ickworth, PC, MP (1696-1743) holding his Purse of Office as Lord Privy Seal

Loo, Jean-Baptiste van (1684-1745)

USB1156579

Warsaw Ghetto Uprising - Photo from Jürgen Stroop Report to Heinrich …, 1945 (photo)

Warsaw Ghetto Uprising - Photo from Jürgen Stroop Report to Heinrich …, 1945 (photo)

Reinhard Schultz

IMO8738210

The Churning of the Ocean of Milk, c.1825 (opaque w/c & gold on paper)

The Churning of the Ocean of Milk, c.1825 (opaque w/c & gold on paper)

Indian School, (19th century)

SD5863973

Emperor Napoleon I Bonaparte (1769-1821) with his son Prince Napoleon Francois Charles Joseph Bonaparte, who became the king of Rome Napoleon II also later called the Aiglon - Napoleon watching the King of Italy (Napoleon II) taking his first steps in a cariage pulled by goats, 1811 - lithograph by Job (Jacques Onfroabout Breville) from “” Le Grand Napoleon of Little Children”” 1893

Emperor Napoleon I Bonaparte (1769-1821) with his son Prince Napoleon Francois Charles Joseph Bonaparte, who became the king of Rome Napoleon II also later called the Aiglon - Napoleon watching the King of Italy (Napoleon II) taking his first steps in a cariage pulled by goats, 1811 - lithograph by Job (Jacques Onfroabout Breville) from “” Le Grand Napoleon of Little Children”” 1893

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Stefano Bianchetti

XEE4160585

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