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Images of 'Bisected' found, 26

Vestige '93--2, 1993 (porcelain with lacquer & Japanese cypress wood (hinoki))
 
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  • Copyright Applies
Vestige '93--2, 1993 (porcelain with lacquer & Japanese cypress wood (hinoki))

Yagi Akira (b.1955)

FSG5617294

Vestige '93--2, 1993 (porcelain with lacquer & Japanese cypress wood (hinoki))

Yagi Akira (b.1955)

FSG5617294

Transit Circle, Greenwich
 
Transit Circle, Greenwich

XLF3792684

Transit Circle, Greenwich

XLF3792684

False window bisected by columns which give illusion of chandeliers, work by Giovanni Antonio Amadeo (1447-1522), facade, Certosa di Pavia, Italy, 16th century
 
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  • Permission required for immersive exhibition use - Please contact us;Permission required for TV use - Please contact us
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  • Bridgeman Images only provides access to this image. Consent to use and possible payment of an additional fee may be required according to Italian Cultural Heritage Code and would need to be cleared in advance with the institution where the work is kept.
False window bisected by columns which give illusion of chandeliers, work by Giovanni Antonio Amadeo (1447-1522), facade, Certosa di Pavia, Italy, 16th century

DGA755416

False window bisected by columns which give illusion of chandeliers, work by Giovanni Antonio Amadeo (1447-1522), facade, Certosa di Pavia, Italy, 16th century

DGA755416

Richmond Park, Greater London: the trunk of a mature tree, split in half down to the ground, 1962-64 (b/w photo)
 
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Richmond Park, Greater London: the trunk of a mature tree, split in half down to the ground, 1962-64 (b/w photo)

Gay, John (1909-99)

EHT808423

Richmond Park, Greater London: the trunk of a mature tree, split in half down to the ground, 1962-64 (b/w photo)

Gay, John (1909-99)

EHT808423

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Image made with an amateur instrument, a 130 mm bezel. NGC 891 is a classic example of an edge - on galaxy bisected by a dark lane. It is actually a spiral galaxy seen edge - on from the side, so it's spiral structure is hidden from our line of sight. Recent observations indicate that NGC 891 may actually be a barred spiral galaxy, making it an SBB galaxy according to Hubble classification type
 
Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Image made with an amateur instrument, a 130 mm bezel. NGC 891 is a classic example of an edge - on galaxy bisected by a dark lane. It is actually a spiral galaxy seen edge - on from the side, so it's spiral structure is hidden from our line of sight. Recent observations indicate that NGC 891 may actually be a barred spiral galaxy, making it an SBB galaxy according to Hubble classification type

Jerry Lodriguss

PIX4609457

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Image made with an amateur instrument, a 130 mm bezel. NGC 891 is a classic example of an edge - on galaxy bisected by a dark lane. It is actually a spiral galaxy seen edge - on from the side, so it's spiral structure is hidden from our line of sight. Recent observations indicate that NGC 891 may actually be a barred spiral galaxy, making it an SBB galaxy according to Hubble classification type

Jerry Lodriguss

PIX4609457

Nebulae M20 - M8 in Sagittarius - M20 and M8 nebulas in Sagittarius - View of nebulae of the Lagoon (M8/NGC 6523), below, and Trifide (M20), above. Located in Sagittarius, these nebulae are about 5000 light years away from Earth. From a dark site, the Lagoon nebula (M8), bottom, is visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. Taking its name from the dark lane that runs through the center of the nebula, just to the west of open cluster NGC 6530, the Lagoon nebula is a beautiful sight in any size telescope. M20, top, is a spectacular combination of emission and reflection nebulosity, bisected by the dark nebula B85
 
Nebulae M20 - M8 in Sagittarius - M20 and M8 nebulas in Sagittarius - View of nebulae of the Lagoon (M8/NGC 6523), below, and Trifide (M20), above. Located in Sagittarius, these nebulae are about 5000 light years away from Earth. From a dark site, the Lagoon nebula (M8), bottom, is visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. Taking its name from the dark lane that runs through the center of the nebula, just to the west of open cluster NGC 6530, the Lagoon nebula is a beautiful sight in any size telescope. M20, top, is a spectacular combination of emission and reflection nebulosity, bisected by the dark nebula B85

Stephane Guisard

PIX4619767

Nebulae M20 - M8 in Sagittarius - M20 and M8 nebulas in Sagittarius - View of nebulae of the Lagoon (M8/NGC 6523), below, and Trifide (M20), above. Located in Sagittarius, these nebulae are about 5000 light years away from Earth. From a dark site, the Lagoon nebula (M8), bottom, is visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. Taking its name from the dark lane that runs through the center of the nebula, just to the west of open cluster NGC 6530, the Lagoon nebula is a beautiful sight in any size telescope. M20, top, is a spectacular combination of emission and reflection nebulosity, bisected by the dark nebula B85

Stephane Guisard

PIX4619767

Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula
 
Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula

PIX4622466

Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula

PIX4622466

Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula
 
Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula

R. Gendler

PIX4622441

Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula

R. Gendler

PIX4622441

Elliptical Galaxy Centaurus A (NGC 5128) - The galaxy Centaurus A - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. This giant galaxy is a powerful radio source known as Centaurus A. The central dark band would be the rest of dust in a spiral galaxy smaller than the giant galaxy would have cannibalized. Centaurus A is an active galaxy whose energy comes from a supermassive black hole. Image made with an amateur instrument, a 130 mm bezel. Designated as radio source Centaurus A, NGC 5128 is one of the most peculiar galaxies in the sky. It is bisected by a dark lane that is considered the dust remnant of a smaller spiral galaxy that was cannibalized by the larger elliptical galaxy. The collision resulted in a burst of star formation. A gigantic black hole equivalent to one billion solar masses resides inside NGC 5128
 
Elliptical Galaxy Centaurus A (NGC 5128) - The galaxy Centaurus A - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. This giant galaxy is a powerful radio source known as Centaurus A. The central dark band would be the rest of dust in a spiral galaxy smaller than the giant galaxy would have cannibalized. Centaurus A is an active galaxy whose energy comes from a supermassive black hole. Image made with an amateur instrument, a 130 mm bezel. Designated as radio source Centaurus A, NGC 5128 is one of the most peculiar galaxies in the sky. It is bisected by a dark lane that is considered the dust remnant of a smaller spiral galaxy that was cannibalized by the larger elliptical galaxy. The collision resulted in a burst of star formation. A gigantic black hole equivalent to one billion solar masses resides inside NGC 5128

Jerry Lodriguss

PIX4612235

Elliptical Galaxy Centaurus A (NGC 5128) - The galaxy Centaurus A - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. This giant galaxy is a powerful radio source known as Centaurus A. The central dark band would be the rest of dust in a spiral galaxy smaller than the giant galaxy would have cannibalized. Centaurus A is an active galaxy whose energy comes from a supermassive black hole. Image made with an amateur instrument, a 130 mm bezel. Designated as radio source Centaurus A, NGC 5128 is one of the most peculiar galaxies in the sky. It is bisected by a dark lane that is considered the dust remnant of a smaller spiral galaxy that was cannibalized by the larger elliptical galaxy. The collision resulted in a burst of star formation. A gigantic black hole equivalent to one billion solar masses resides inside NGC 5128

Jerry Lodriguss

PIX4612235

Chitral Relief camp, 1915 (b/w photo)
 
Chitral Relief camp, 1915 (b/w photo)

UIG1583511

Chitral Relief camp, 1915 (b/w photo)

UIG1583511

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North on Dione is 140 degrees to the left
 
Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

PIX4625507

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

PIX4625507

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the outskirts of the galaxy on a plane perpendicular to the jets. The arcs of multimillion degree gas appear to be part of a projected ring 25,000 light years in diameter. The size and location of the ring indicate that it may have been produced in a titanic explosion that occurred about ten million years ago
 
Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

PIX4612202

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

PIX4612202

Overberg (screenprint)
 
Copyright
  • Copyright Applies
Overberg (screenprint)

Rae, Barbara (b.1943)

LYT6771124

Overberg (screenprint)

Rae, Barbara (b.1943)

LYT6771124

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