Arp 25
One of the many starburst spiral arms contains an intermediate mass black hole with 50,000 times the mass of the Sun, named NGC 2276-3c. NGC 2276-3c has produced two jets: a large-scale radio jet, approximately 2,000 light years long, and an "inner jet" about 6 light years long. The galaxy shows an enhanced rate of star formation that may have been triggered by a collision with a dwarf galaxy, or by the gravitational interaction with its neighbor compressing gas and dust.
NGC 2276 was discovered by Friedrich August Theodor Winnecke on 26 June 1876. In the Atlas of Peculiar Galaxies, the galaxy is mentioned twice, once as Arp 25, in the category spiral galaxies with one heavy arm, and with NGC 2300 as Arp 114, in the category elliptical galaxies close to and perturbing spiral galaxies.
Supernovae
Six supernovae have been observed in NGC 2276:
- SN 1962Q (type unknown, mag. 16.9) was discovered by Shachbazian and Iskudarian on 25 February 1962.
- SN 1968V (type II, mag. 15.7) was discovered by Shachbazian on 26 January 1968.
- SN 1968W (type unknown, mag. 16.6) was discovered by Iskudarian on 24 March 1968.
- SN 1993X (type II, mag. 16.3) was discovered by the Leuschner Observatory Supernova Search on 22 August 1993.
- SN 2005dl (type II, mag. 17.1) was discovered by Alessandro Dimai (bio-it) and Marco Migliardi on 25 August 2005.
- SN 2016gfy (type II, mag. 16.3) was discovered by Alessandro Dimai on 13 September 2016.
Gallery
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HST Image
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The trailing arms of NGC 2276
References
- ^ "Results for object NGC 2276". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 2006-11-18.
- ^ Roberts, I. D.; Van Weeren, R. J.; De Gasperin, F.; Botteon, A.; Edler, H. W.; Ignesti, A.; Matijević, L.; Tomičić, N. (2024). "A 100 kpc ram pressure tail trailing the group galaxy NGC 2276". Astronomy & Astrophysics. 689: A22. arXiv:2406.09221. Bibcode:2024A&A...689A..22R. doi:10.1051/0004-6361/202450672.
- ^ "NGC 2276: NASA's Chandra Finds Intriguing Member of Black Hole Family Tree". Chandra X-ray Center. Retrieved 2 January 2016.
- ^ Harbaugh, Jennifer (2015-02-26). "NASA's Chandra Finds Intriguing Member of Black Hole Family Tree". NASA. Retrieved 2 January 2016.
- ^ Seligman, Courtney. "New General Catalogue Objects: NGC 2276". Celestial Atlas. Retrieved 29 December 2024.
- ^ "SN 1962Q". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ Barbon, R.; Buondí, V.; Cappellaro, E.; Turatto, M. (1999). "The Asiago Supernova Catalogue - 10 years after". Astronomy and Astrophysics Supplement Series. 139 (3): 531. arXiv:astro-ph/9908046. Bibcode:1999A&AS..139..531B. doi:10.1051/aas:1999404.
- ^ "SN 1968V". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ "SN 1968W". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ Treffers, R. R.; Filippenko, A. V.; Leibundgut, B.; Paik, Y.; Lee, L. F. M.; Richmond, M. W. (1993). "Supernova 1993X in NGC 2276". International Astronomical Union Circular (5850): 1. Bibcode:1993IAUC.5850....1T.
- ^ "SN 1993X". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ Dimai, A.; Migliardi, M.; Manzini, F. (2005). "Supernova 2005dl in NGC 2276". International Astronomical Union Circular (8588): 2. Bibcode:2005IAUC.8588....2D.
- ^ "SN 2005dl". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ "SN 2016gfy". Transient Name Server. IAU. Retrieved 29 December 2024.
- ^ "Hubble Inspects a Contorted Spiral Galaxy". Retrieved June 8, 2021.
External links
- Supernova SN 2016gfy in NGC 2276 from The Virtual Telescope Project
- NGC 2276 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images