NGC 1023
| NGC 1023 | |
|---|---|
 Barred lenticular galaxy NGC 1023 | |
| Observation data (J2000 epoch) | |
| Constellation | Perseus |
| Right ascension | 02h 40m 24.0s[1] |
| Declination | +39° 03′ 48″[1] |
| Redshift | 0.002125[1] |
| Helio radial velocity | 637 ± 4 km/s[1] |
| Distance |
~19 Mly (Light Travel-Time redshift-based)[1] 30 to 64 Mly (measured)[1] |
| Apparent magnitude (V) | 10.35[1] |
| Characteristics | |
| Type | SB0[1] |
| Apparent size (V) | 8.7' x 3.0'[1] |
| Other designations | |
| UGC 2154, PGC 10123, MCG+06-06-073, Arp 135 | |
NGC 1023 is a barred lenticular galaxy, a member of the NGC 1023 group of galaxies in the Local Supercluster. Distance measurements vary from 9.3 to 19.7 million parsecs (30 to 64 million light-years).[1] The supermassive black hole at the core has a mass of (4.4±0.5)×107 M☉.[2]
NGC 1023 is included in Halton Arp's Atlas of Peculiar Galaxies, under the category "Galaxies with Nearby Fragments" under the number 135.[3]
References
- 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 1023. Retrieved 2012-10-17.
- ↑ Graham, Alister W. (November 2008), "Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values", Publications of the Astronomical Society of Australia, 25 (4): 167–175, arXiv:0807.2549, Bibcode:2008PASA...25..167G, doi:10.1071/AS08013.
- ↑ Arp, Halton (1966). Atlas of Peculiar Galaxies. Pasadena, California: California Institute of Technology. Retrieved 5 Jan 2010. (webpage includes PDF link)
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