NGC 5030
NGC 5030[6] is a barred spiral galaxy in the constellation Virgo. The object was discovered on 17 March 1881 by the American astronomer Edward Singleton Holden.[7]
NGC 5030 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 13h 13m 54.144s[1] |
Declination | −16° 29′ 27.43″[1] |
Redshift | 2397 km/s[2] |
Helio radial velocity | 0.007996[2] |
Distance | 118.7 Mly (36.39 Mpc)[3] |
Apparent magnitude (B) | 14.2[4] |
Characteristics | |
Type | SB0+(r)?[5] |
Size | 56,500 ly (17,330 pc)[2][note 1] |
Apparent size (V) | 1.8′ × 1.3′[2] |
Other designations | |
NGC 5030, MCG-03-34-023, PGC 45991[5] |
See also
References
- Skrutskie, M.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
- "NED results for object NGC 5030". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 14 May 2018.
- Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201.
- Mendel, J. Trevor; Proctor, Robert N; Forbes, Duncan A; Brough, Sarah (2008). "The anatomy of the NGC 5044 group - I. Group membership and dynamics". Monthly Notices of the Royal Astronomical Society. 389 (2): 749. arXiv:0806.3127. Bibcode:2008MNRAS.389..749M. doi:10.1111/j.1365-2966.2008.13514.x.
- "NGC 5030". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 10 May 2018.
- "Revised NGC Data for NGC 5030". spider.seds.org. Retrieved 2018-04-13.
- Seligman, Courtney. "New General Catalogue objects: NGC 5000 - 5049". cseligman.com. Retrieved 14 May 2018.
Notes
- RC3 D25; R25 (blue) values used.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.