NGC 605
NGC 605 is a lenticular galaxy in the constellation Andromeda, which is about 234 million light-years from the Milky Way. It was discovered on October 21, 1881 by the French astronomer Édouard Jean-Marie Stephan.[6][5]
| NGC 605 | |
|---|---|
 NGC 605 | |
| Observation data (J2000 epoch) | |
| Constellation | Andromeda |
| Right ascension | 01h 35m 02.34063s[1] |
| Declination | +41° 14′ 53.3204″[1] |
| Redshift | 0.01705±0.00010[2] |
| Helio radial velocity | 5,110.86±29.98[2] |
| Distance (comoving) | 233.6 ± 16.4 Mly (71.63 ± 5.04 Mpc)[2] |
| Characteristics | |
| Type | S0[3] |
| Apparent size (V) | 0.827 × 0.496 arcmin[4] |
| Other designations | |
| UGC 1128[5] | |
References
- 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.
- Huchra, John P.; et al. (April 1999). "The CFA Redshift Survey: Data for the South Galactic CAP". The Astrophysical Journal Supplement Series. 121 (2): 287–368. Bibcode:1999ApJS..121..287H. doi:10.1086/313194.
- de Vaucouleurs, G.; et al. (1991). "Third reference catalogue of bright galaxies". 3.9. New York: Springer-Verlag. Cite journal requires
|journal=(help) - Skrutskie, M. F.; et al. (February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
- "NGC 605". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-08.
- Ford, Dominic. "The galaxy NGC 605 - In-The-Sky.org". in-the-sky.org. Retrieved 2019-12-12.
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