NGC 2841
Coordinates: 9h 22m 02.6s, +50° 58′ 35″
NGC 2841 | |
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300px
Infrared image derived from data taken by the Spitzer Space Telescope.
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Observation data (J2000 epoch) | |
Constellation | Ursa Major |
Right ascension | 9h 22m 02.6s[1] |
Declination | +50° 58′ 35″[1] |
Redshift | 638 ± 3 km/s[1] |
Type | SA(r)b[1] |
Apparent dimensions (V) | 8′.1 × 3′.5[1] |
Apparent magnitude (V) | 10.1[1] |
Other designations | |
UGC 4966, PGC 26512[1] | |
NGC 2841 is an inclined unbarred spiral galaxy in the constellation Ursa Major. Initially thought to be about 30 million light years distant, a 2001 Hubble Space Telescope survey of the galaxy's Cepheid variables determined that it was approximately 14.1 megaparsecs or 46 million light years distant.[2]
Structure
Structurally, NGC 2841 is a giant spiral galaxy with properties similar to those of the Andromeda Galaxy.[2] It is a prototypical flocculent spiral galaxy, a type of spiral galaxy whose arms are patchy and discontinuous.[3]
NGC 2841 is also noted for its large population of young blue stars, and few H II regions.[4]
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NGC2841HunterWilson.jpg
Amateur Image of NGC 2841.
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Hubble image of NGC 2841.
LINER emission
NGC 2841 contains a low-ionization nuclear emission-line region (LINER), a type of region that is characterized by spectral line emission from weakly ionized atoms.[5]
See also
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Wikimedia Commons has media related to Lua error in package.lua at line 80: module 'strict' not found.. |
- NGC 2841 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
References
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- ↑ "A Near-Infrared Atlas of Spiral Galaxies", Debra Meloy Elmegreen, "CH3. Discussion" (accessed 23 April 2010)
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