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NGC 262 (also known as Markarian 348) is the largest known spiral galaxy, [5] located in the constellation Andromeda. [1] It is a Seyfert 2 spiral galaxy located 287 million light years away. [2] It was discovered on 17 September 1885 by Lewis A. Swift. [4] According to A.M. Garcia, NGC 262 is a member of the NGC 315 Group (also known as LGG 14).
Nebula Maximum dimension (in light-years/parsecs) Type Notes NGC 262 Halo Cloud 1,300,000 ly (400,000 pc) [1] H I region: Spiral nebula surrounding NGC 262, which is one of the largest known galaxies. Leo Ring: 650,000 ly (200,000 pc) [2] HVC: A large ring of cold gas that formed from a collision of two galaxies. [3] Magellanic Stream
NGC 2626 is a reflection nebula, emission nebula, and absorption nebula in the constellation Vela. [ 4 ] [ 5 ] It is mostly illuminated by B1 star CD-40 4432 and ionized by the O8 quadruple star system HD 73882 , together with other stars.
Sharpless 101, Cygnus Star Cloud 105: Crescent Nebula: Sh2 105, NGC 6888, Sharpless 105, Caldwell 27 106: Celestial Snow Angel: Sh2-106, Celestial Snow Angel 117: North America Nebula: NGC 7000, Caldwell 20 125: Cocoon Nebula: IC 5146, Caldwell 19 140: Sh2-140: Sh2-140 155: Cave Nebula: Sh2-155, Caldwell 9 158: NGC 7538: Sh2-158, NGC 7538 162 ...
NGC 2022 is a planetary nebula in the equatorial constellation of Orion, located at a distance of 8.21 kilolight-years from the Sun. [3] It was first observed by William Herschel on December 28, 1785, who described it as: considerably bright, nearly round, like a star with a large diameter, like an ill-defined planetary nebula. [7]
The cone's shape comes from a dark absorption nebula consisting of cold molecular hydrogen and dust in front of a faint emission nebula containing hydrogen ionized by S Monocerotis, the brightest star of NGC 2264. The faint nebula is approximately seven light-years long (with an apparent length of 10 arcminutes), and is 2,700 light-years from ...
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The molecular cloud is located about 1400 light-years away in the L1630 dark cloud, which is part of the Orion B molecular cloud in the constellation of Orion. [3] [4] The region contains multiple protostars (two class 0 and one class I) and four more evolved IRAS sources. The three protostars are driving the Herbig-Haro objects in this region. [3]