UGC 5081, CGCG 063-001,MCG +02-25-001,PGC 27074[1]
NGC 2906 is aspiral galaxy in the constellationLeo. It is circa 120 millionlight years from Earth, which, given its apparent dimensions, means that NGC 2906 is about 75,000 light years across. It was discovered byWilliam Herschel on December 28, 1785.[3]
The galaxy is characterised by a normalstar formation rate,[4] which has been calculated to be 0.8M☉ per year. The total mass of the galaxy is estimated to be4×1010M☉.[5] A total of 241HII regions have been identified in the galaxy.[6]
Onesupernova has been observed in NGC 2906,SN 2005ip. The supernova was discovered by T. Boles on November 6, 2005, with a 0.35m refractor, with an estimated apparent magnitude 15.5 and was identified as atype II supernova, probably within a few weeks past explosion.[7] As the supernova declined in brightness, it reached a plateau that lasted for a bit more than two years and itsspectrum became dominated by narrow lines (IIn), an unusual feature of supernovae, that was attributed to the interaction of the supernova with dust located around it.[8] It is also possible that the supernova created dust.[9]
NGC 2906 is member of agroup of galaxies, the NGC 2894 group. Other galaxies identified as members of the cluster areNGC 2882,NGC 2894, and IC 450.[10]
^Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P.; García-Benito, R.; Ibarra-Mede, H. J.; González, J. J.; Rosales-Ortega, F. F.; Sánchez-Menguiano, L.; Ascasibar, Y.; Bitsakis, T.; Law, D.; Cano-Díaz, M.; López-Cobá, C.; Marino, R. A.; Gil de Paz, A.; López-Sánchez, A. R.; Barrera-Ballesteros, J.; Galbany, L.; Mast, D.; Abril-Melgarejo, V.; Roman-Lopes, A. (April 2016). "Pipe3D, a pipeline to analyze Integral Field Spectroscopy Data: II. Analysis sequence and CALIFA dataproducts".Revista Mexicana de Astronomía y Astrofísica.52:171–220.arXiv:1602.01830.Bibcode:2016RMxAA..52..171S.
^Smith, Nathan; Silverman, Jeffrey M.; Chornock, Ryan; Filippenko, Alexei V.; Wang, Xiaofeng; Li, Weidong; Ganeshalingam, Mohan; Foley, Ryan J.; Rex, Jacob; Steele, Thea N. (20 April 2009). "Coronal lines and dust formation in SN 2005ip: not the brightest, but the hottest type IIn supernova".The Astrophysical Journal.695 (2):1334–1350.arXiv:0809.5079.Bibcode:2009ApJ...695.1334S.doi:10.1088/0004-637X/695/2/1334.S2CID15737210.
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