Galaxy in the constellation Sculptor
NGC 612 is a lenticular galaxy in the constellation of Sculptor located approximately 388 million light-years from Earth. It is a type II Seyfert galaxy and thus has an active galactic nucleus.[1][4] NGC 612 has been identified as an extremely rare example of a non-elliptical radio galaxy, hosting one of the nearest powerful FR-II radio sources.[6][7]
- ^ a b c d e f g "NGC 612 NASA/IPAC Extragalactic Database Results". ned.ipac.caltech.edu. Retrieved 2018-10-31.
- ^ Cite error: The named reference
professor
was invoked but never defined (see the help page).
- ^ Ruffa, Ilaria; Davis, Timothy A.; Cappellari, Michele; Bureau, Martin; Elford, Jacob; Iguchi, Satoru; Lelli, Federico; Liang, Fu-Heng; Liu, Lijie; Lu, Anan; Sarzi, Marc; Williams, Thomas G. (2023). "WISDOM project – XIV. SMBH mass in the early-type galaxies NGC 0612, NGC 1574, and NGC 4261 from CO dynamical modelling". Monthly Notices of the Royal Astronomical Society. 522 (4): 6170–6195. arXiv:2304.06117. Bibcode:2023MNRAS.522.6170R. doi:10.1093/mnras/stad1119.
- ^ a b "Revised NGC Data for NGC 612". spider.seds.org. Retrieved 2018-10-31.
- ^ "NGC 612". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-19.
- ^ Véron-Cetty, M. P.; Véron, P. (2001). "Are all radio galaxies genuine ellipticals?". Astronomy & Astrophysics. 375 (3): 791–796. Bibcode:2001A&A...375..791V. doi:10.1051/0004-6361:20010902. ISSN 0004-6361.
- ^ Emonts, B. H. C.; Morganti, R.; Oosterloo, T. A.; Holt, J.; Tadhunter, C. N.; van der Hulst, J. M.; Ojha, R.; Sadler, E. M. (2008). "Enormous disc of cool gas surrounding the nearby powerful radio galaxy NGC 612 (PKS 0131−36)". Monthly Notices of the Royal Astronomical Society. 387 (1): 197–208. arXiv:0805.3371. Bibcode:2008MNRAS.387..197E. doi:10.1111/j.1365-2966.2008.13142.x. ISSN 0035-8711. S2CID 7916786.