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'Expulsion' Bilder und Clips Suchergebnisse page 2881 of 33

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Bilder zu 'Expulsion' gefunden, 2,903

 
Korea: At Jaengung Brothel. Shin Yun-bok (1758-?), 1805

PFH2562366

Korea: At Jaengung Brothel. Shin Yun-bok (1758-?), 1805

PFH2562366

 
Korea: Going to the temple. Shin Yun-bok (1758-?), 1805

PFH2562365

Korea: Going to the temple. Shin Yun-bok (1758-?), 1805

PFH2562365

 
Galaxy M82 in the Great Bear seen in X-rays - The galaxy M82 seen in X-ray - Image obtained by Chandra in X-rays, reveals a cloud (in red) of very hot gas of several million degres emitted from the central regions of the galaxy. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Chandra's X - ray image reveals gas that has been heated to millions of degrees by the violent outflow of matter blasting out of the galaxy. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy. Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss f

PIX4610440

Galaxy M82 in the Great Bear seen in X-rays - The galaxy M82 seen in X-ray - Image obtained by Chandra in X-rays, reveals a cloud (in red) of very hot gas of several million degres emitted from the central regions of the galaxy. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Chandra's X - ray image reveals gas that has been heated to millions of degrees by the violent outflow of matter blasting out of the galaxy. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy. Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss f

PIX4610440

 
Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Hubble Space Telescope (HST). The colors used in this image correspond to the emissions of different gases: sulfur in green, hydrogen in orange and oxygen in blue. Hubble Space Telescope have photographed a festive - looking nearby planetary nebula called NGC 5189. Planetary nebulae represent the final brief stage in the life of a medium - sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material then becomes heated by the radiation from the stellar remnant and radiates, producing glowing clouds of gas that can show complex structures, as the ejection of mass from the star is uneven in both time and direction. This image was taken with Hubble's Wide Field Camera 3 on October 8, 2012, in filters tuned to

PIX4623125

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Hubble Space Telescope (HST). The colors used in this image correspond to the emissions of different gases: sulfur in green, hydrogen in orange and oxygen in blue. Hubble Space Telescope have photographed a festive - looking nearby planetary nebula called NGC 5189. Planetary nebulae represent the final brief stage in the life of a medium - sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material then becomes heated by the radiation from the stellar remnant and radiates, producing glowing clouds of gas that can show complex structures, as the ejection of mass from the star is uneven in both time and direction. This image was taken with Hubble's Wide Field Camera 3 on October 8, 2012, in filters tuned to

PIX4623125

 
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Baltimore City Jail Riots, 1972

MOV8613839

Baltimore City Jail Riots, 1972

MOV8613839

 
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Psalter, Gallican version. Large historiated initial 'B', containing Tree of Jesse. in medallions in lower and outer borders, beginning bottom 1 .: - (i) The Almighty between cherubim. (ii) Creation of Eve; Hellmouth on 1 . (iii) The Almighty warning Adam and Eve, and the Fall. (iv) Adam and Eve hiding from the Almighty, and the Expulsion. (v) Adam digging, Eve spinning; offerings of Cain and Abel, and death of Abel. (vi) Lamech killing Cain, and death of the boy Jabal. (vii) Building of the Ark. (viii) Noah and family entering the Ark; outside, the raven feeding on dead horse. (ix) Drunkenness of Noah. These borders contain also minute figures, animals, birds, insects, and foliage of extraordinary delicacy, and at the top of the lower border are two medallions of a knight and his lady, the former on r . having the arms of the St. Omer family.

BL3296712

Psalter, Gallican version. Large historiated initial 'B', containing Tree of Jesse. in medallions in lower and outer borders, beginning bottom 1 .: - (i) The Almighty between cherubim. (ii) Creation of Eve; Hellmouth on 1 . (iii) The Almighty warning Adam and Eve, and the Fall. (iv) Adam and Eve hiding from the Almighty, and the Expulsion. (v) Adam digging, Eve spinning; offerings of Cain and Abel, and death of Abel. (vi) Lamech killing Cain, and death of the boy Jabal. (vii) Building of the Ark. (viii) Noah and family entering the Ark; outside, the raven feeding on dead horse. (ix) Drunkenness of Noah. These borders contain also minute figures, animals, birds, insects, and foliage of extraordinary delicacy, and at the top of the lower border are two medallions of a knight and his lady, the former on r . having the arms of the St. Omer family.

BL3296712

 
Germany: Henry IV (1050-1106), 18th Holy Roman emperor, 1645 (engraving)

PFH5302947

Germany: Henry IV (1050-1106), 18th Holy Roman emperor, 1645 (engraving)

PFH5302947

 
Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

PIX4623552

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

PIX4623552

 
Proto - planetary nebula OH231.8+4.2 dans la Poupe/HST

PIX4623703

Proto - planetary nebula OH231.8+4.2 dans la Poupe/HST

PIX4623703

 
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

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

PIX4623752

 
Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

PIX4623194

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

PIX4623194

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Indians involved in the the Hindu-German Conspiracy Trial which commenced in the District Court in San Francisco on November 12, 1917 following the uncovering of the Hindu-German Conspiracy (also known as the Indo German plot) for initiating a revolt in India. It was part of a wave of such incidents which took place in the United States after America's entrance into World War I. In May 1917, eight Indian nationalists of the Ghadar Party were indicted by a federal grand jury on a charge of conspiracy to form a military enterprise against the United Kingdom. The trial lasted from November 20, 1917 to April 24, 1918. The British authorities hoped that the conviction of the Indians would result in their deportation from the United States back to India. However, strong public support in favor of the Indians meant that the U.S. Department of Justice chose not to do so. The trial ended with a sensational climax when Ram Chandra was shot to death in the courtroom by fellow defendant, Ram Sing

BL3292013

Indians involved in the the Hindu-German Conspiracy Trial which commenced in the District Court in San Francisco on November 12, 1917 following the uncovering of the Hindu-German Conspiracy (also known as the Indo German plot) for initiating a revolt in India. It was part of a wave of such incidents which took place in the United States after America's entrance into World War I. In May 1917, eight Indian nationalists of the Ghadar Party were indicted by a federal grand jury on a charge of conspiracy to form a military enterprise against the United Kingdom. The trial lasted from November 20, 1917 to April 24, 1918. The British authorities hoped that the conviction of the Indians would result in their deportation from the United States back to India. However, strong public support in favor of the Indians meant that the U.S. Department of Justice chose not to do so. The trial ended with a sensational climax when Ram Chandra was shot to death in the courtroom by fellow defendant, Ram Sing

BL3292013

 
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Sinn Fein Prisoners, 1916

IWF7405567

Sinn Fein Prisoners, 1916

IWF7405567

 
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Oslo 1984-01-23: Treholt case. On January 23, 1984, agency manager Arne Treholt …, 1984 (photo)

Henrik Laurvik

NTB8964755

Oslo 1984-01-23: Treholt case. On January 23, 1984, agency manager Arne Treholt …, 1984 (photo)

Henrik Laurvik

NTB8964755

 
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Portugal. Birth of freedom, 1974

MOD6437291

Portugal. Birth of freedom, 1974

MOD6437291

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