NGC 2552

NGC 2552
NGC 2552
	SDSS image of NGC 2552
Observation data (J2000 epoch)
Constellation	Lynx
Right ascension	08h 19m 19.58s
Declination	50° 00′ 20.8″
Distance	22 Mly (6.7 Mpc)
Characteristics
Type	SA(s)m
Other designations
	UGC 4325, PGC 23340

NGC 2552 is a Magellanic spiral galaxy located some 22^[2] million light years away. It can be found in constellation of Lynx. This is a type of unbarred dwarf galaxy, usually with a single spiral arm. It is inclined by 41° to the line of sight from the Earth along a position angle of 229°.^[2] The measured velocity dispersion of the stars in NGC 2552 is relatively low—a mere 19 ± 2 km/s.^[3] This galaxy forms part of a loose triplet that includes NGC 2541 and NGC 2500, which together belong to the NGC 2841 group.^[4]

References

^ Adelman-McCarthy, J. K.; et al. (March 2007), "The SDSS Photometric Catalog, Release 5", VizieR On-line Data Catalog: II/276, Bibcode:2007yCat.2276....0A.
^ ^a ^b ^c ^d ^e Garrido, O.; et al. (June 2002), "GHASP: An Hα kinematic survey of spiral and irregular galaxies. I. Velocity fields and rotation curves of 23 galaxies", Astronomy & Astrophysics, 387 (3): 821–829, arXiv:1304.4176, Bibcode:2002A&A...387..821G, doi:10.1051/0004-6361:20020479, S2CID 122952094.
^ Hunter, Deidre A.; et al. (November 2002), "The Stellar and Gas Kinematics of Several Irregular Galaxies", Astronomy & Astrophysics, 580 (1): 194–212, arXiv:astro-ph/0207510, Bibcode:2002ApJ...580..194H, doi:10.1086/343080, S2CID 17572211.
^ Ferrarese, Laura; et al. (May 29, 1998), "The HST Key Project on the Extragalactic Distance Scale XII. The Discovery of Cepheids and a New Distance to NGC 2541", The Astrophysical Journal, 507 (2): 655–690, arXiv:astro-ph/9805365, Bibcode:1998ApJ...507..655F, doi:10.1086/306364, S2CID 204935980.

External links

Media related to NGC 2552 at Wikimedia Commons
astronomerica.awardspace.com NGC2552 Archived 2011-02-26 at the Wayback Machine image
NGC 2552 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

This spiral galaxy article is a stub. You can help Wikipedia by expanding it.

[AdelmanMcCarthy2007-1] Adelman-McCarthy, J. K.; et al. (March 2007), "The SDSS Photometric Catalog, Release 5", VizieR On-line Data Catalog: II/276, Bibcode:2007yCat.2276....0A.

[AAA387_821-2] Garrido, O.; et al. (June 2002), "GHASP: An Hα kinematic survey of spiral and irregular galaxies. I. Velocity fields and rotation curves of 23 galaxies", Astronomy & Astrophysics, 387 (3): 821–829, arXiv:1304.4176, Bibcode:2002A&A...387..821G, doi:10.1051/0004-6361:20020479, S2CID 122952094.

[AAA580_1_194-3] Hunter, Deidre A.; et al. (November 2002), "The Stellar and Gas Kinematics of Several Irregular Galaxies", Astronomy & Astrophysics, 580 (1): 194–212, arXiv:astro-ph/0207510, Bibcode:2002ApJ...580..194H, doi:10.1086/343080, S2CID 17572211.

[arxiv9805365-4] Ferrarese, Laura; et al. (May 29, 1998), "The HST Key Project on the Extragalactic Distance Scale XII. The Discovery of Cepheids and a New Distance to NGC 2541", The Astrophysical Journal, 507 (2): 655–690, arXiv:astro-ph/9805365, Bibcode:1998ApJ...507..655F, doi:10.1086/306364, S2CID 204935980.

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