NGC 625
NGC 625 is a dwarf barred spiral galaxy about 12.7 Mly away in the constellation Phoenix. It was discovered on 2 September 1826 by Scottish astronomer James Dunlop. NGC 625 is a member of the Sculptor Group.
NGC 625 has an active galactic nucleus, i.e. a compact region at the center that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
See also
References
- ^ "NASA/IPAC Extragalactic Database". Results for NGC 625. Retrieved 2006-12-19.
- ^ Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics. 49 (1): 3–18. Bibcode:2006Ap.....49....3K. doi:10.1007/s10511-006-0002-6. S2CID 120973010.
- ^ Seligman, Courtney. "New General Catalogue Objects: NGC 625". Celestial Atlas. Retrieved 29 August 2024.
- ^ Cannon, John M; et al. (2003). "The Recent Evolution of the Dwarf Starburst Galaxy NGC 625 from Hubble Space Telescope Imaging". The Astronomical Journal. 126 (6): 2806–2830. arXiv:astro-ph/0309542. Bibcode:2003AJ....126.2806C. doi:10.1086/379671. S2CID 15136230.
- ^ "NGC 625". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 August 2024.
External links
- Media related to NGC 625 at Wikimedia Commons
- NGC 625 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images