| NGC 7592 | |
|---|---|
 Hubble Space Telescope (HST) image of the galaxy | |
| Observation data (J2000 epoch) | |
| Constellation | Aquarius |
| Right ascension | 23h 18m 22.2s[1] |
| Declination | −04° 25′ 01″[1] |
| Redshift | 0.024444 ± 0.000113 |
| Heliocentric radial velocity | 7,328 ± 34 km/s[1] |
| Distance | 306 Mly (95 Mpc)[1] |
| Apparent magnitude (V) | 13.5[2] |
| Characteristics | |
| Type | S0+ pec[1] |
| Apparent size (V) | 1.2′ × 0.9′[1] |
| Notable features | mergering galaxy pair |
| Other designations | |
| MCG -01-59-017, VV 731, PGC 70999,[1] Mrk 928 | |
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NGC 7592 is an interacting galaxy system located 300 million light years away in the constellation Aquarius. It was discovered by William Herschel on September 20, 1784.[3] The total infrared luminosity is 1011.33 L☉, and thus it is categorised as a luminous infrared galaxy.[4] One of the galaxies hosts a type 2 Seyfert nucleus.[5]
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 7592. Retrieved 2020-11-03.
- ^ "Revised NGC Data for NGC 7592". spider.seds.org. Retrieved 25 November 2018.
- ^ Seligman, Courtney. "NGC 7592 (= PGC 70999)". Celestial Atlas. Retrieved 19 November 2018.
- ^ Sanders, D. B.; Mazzarella, J. M.; Kim, D.-C.; Surace, J. A.; Soifer, B. T. (October 2003). "The IRAS Revised Bright Galaxy Sample". The Astronomical Journal. 126 (4): 1607–1664. arXiv:astro-ph/0306263. Bibcode:2003AJ....126.1607S. doi:10.1086/376841. S2CID 14825701.
- ^ Maia, Marcio A. G.; Machado, Rodolfo S.; Willmer, Christopher N. A. (October 2003). "The Seyfert Population in the Local Universe". The Astronomical Journal. 126 (4): 1750–1762. arXiv:astro-ph/0307180. Bibcode:2003AJ....126.1750M. doi:10.1086/378360. S2CID 12785006.