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Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border...
Editorial (Books, magazines and newspaper) - extended
Print and/or digital. Single use, any size, inside only. Single language only. Single territory rights for trade books; worldwide rights for academic books. Print run up to 5000. 7 years. (excludes advertising)
$175.00
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$100.00
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Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light years. Aldebaran, Alpha Tauri, a bright red star with a magnitude of 0.75 to 0.95, is located at one end of the V, but does not belong to the cluster. The Taurus Molecular Cloud (TMC) is located on the border of the constellations of Taurus and Perseus. It is a large dense area of gas and dust in space made mostly of molecular hydrogen and helium. It is a birth place of stars, which form from the material in the cloud. Covering about 20 x 30 degrees, this wide - angle image shows a complex of bright red emission nebulae, star clusters, blue reflection nebulosity, and complex dark nebulae. The TMC is located about 400 light years away, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), a very large red emission nebula, is at upper right. Emission nebulae are made up of glowing hydrogen gas. Located in
Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light years. Aldebaran, Alpha Tauri, a bright red star with a magnitude of 0.75 to 0.95, is located at one end of the V, but does not belong to the cluster. The Taurus Molecular Cloud (TMC) is located on the border of the constellations of Taurus and Perseus. It is a large dense area of gas and dust in space made mostly of molecular hydrogen and helium. It is a birth place of stars, which form from the material in the cloud. Covering about 20 x 30 degrees, this wide - angle image shows a complex of bright red emission nebulae, star clusters, blue reflection nebulosity, and complex dark nebulae. The TMC is located about 400 light years away, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), a very large red emission nebula, is at upper right. Emission nebulae are made up of glowing hydrogen gas. Located in
