| NGC 5473 | |
|---|---|
|  SDSS image of NGC 5473 | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major | 
| Right ascension | 14h 04m 43.22677s[1] | 
| Declination | +54° 53′ 33.5103″[1] | 
| Redshift | 0.006558[2] | 
| Heliocentric radial velocity | 1960 km/s[2] | 
| Distance | 85 Mly (26.2 Mpc)[3] | 
| Apparent magnitude (V) | 11.47[4] | 
| Apparent magnitude (B) | 12.37[4] | 
| Characteristics | |
| Type | SAB0−(s):[5] | 
| Other designations | |
| UGC 9011, MCG +09-23-031, PGC 50191[2] | |
NGC 5473 is a lenticular galaxy in the constellation Ursa Major. It was discovered on April 14, 1789 by the astronomer William Herschel.[6] Located roughly 85 million light-years (26.2 megaparsecs) away, it is part of a small galaxy group including NGC 5475 and NGC 5485.[3]
References
- 1 2 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- 1 2 3 "NGC 5473". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-05-06.
- 1 2 Hudson, Michael J.; Robison, Bailey (2018). "The correlation between the sizes of globular cluster systems and their host dark matter haloes". Monthly Notices of the Royal Astronomical Society. 477 (3): 3869–3885. arXiv:1707.02609. doi:10.1093/mnras/sty844.
- 1 2 "Search specification: NGC 5473". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-05-06.
- ↑ "Results for object NGC 5473 (NGC 5473)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-05-06.
- ↑ Seligman, Courtney. "New General Catalogue objects: NGC 5450 - 5499". cseligman.com. Retrieved 2021-05-06.
External links
 Media related to NGC 5473 at Wikimedia Commons
 Media related to NGC 5473 at Wikimedia Commons
    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.
