NGC 5806
Coordinates: 15h 00m 00.40s, +1° 53′ 27″
NGC 5806 | |
---|---|
| |
Observation data (J2000 epoch) | |
Constellation | Virgo[1] |
Right ascension | 15h 00m 00.40s[2] |
Declination | +1° 53′ 27″[1] |
Redshift | 0.004533[1] |
Distance | 69.76 million lightyears[1] |
Type | SBb |
Apparent magnitude (V) | 11.7[1] |
NGC 5806 is a barred spiral galaxy in the constellation Virgo.[2][1]
Supernova Imposter
NGC 5806 contains a star that was catalogued as a supernova (SN Hunt 248), but turned out to be a supernova imposter. The progenitor was detected as a cool hypergiant with an absolute visual magnitude of −9 and 400,000 times more luminous than the sun. The eruption saw it increase in luminosity to around 80,000,000 L☉.[3]
Supernova
NGC 5806 has also hosted a true supernova, SN 2004dg, around 100 times brighter than SN Hunt 248. This was a typical type II supernova. The progenitor has not been detected and is expected to have been a relatively low mass, low luminosity, red supergiant.[4]
References
- 1 2 3 4 5 6 "NGC 5806". Retrieved December 8, 2011.
- 1 2 "Galaxy NGC 5806". Retrieved December 8, 2011.
- ↑ Mauerhan, Jon C.; Van Dyk, Schuyler D.; Graham, Melissa L.; Zheng, Weikang; Clubb, Kelsey I.; Filippenko, Alexei V.; Valenti, Stefano; Brown, Peter; Smith, Nathan; Howell, D. Andrew; Arcavi, Iair (2015). "SN Hunt 248: A super-Eddington outburst from a massive cool hypergiant". Monthly Notices of the Royal Astronomical Society 447 (2): 1922. arXiv:1407.4681. Bibcode:2015MNRAS.447.1922M. doi:10.1093/mnras/stu2541.
- ↑ Smartt, S. J.; Eldridge, J. J.; Crockett, R. M.; Maund, J. R. (2009). "The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae". Monthly Notices of the Royal Astronomical Society 395 (3): 1409. arXiv:0809.0403. Bibcode:2009MNRAS.395.1409S. doi:10.1111/j.1365-2966.2009.14506.x.
External Links
Wikimedia Commons has media related to NGC 5806. |
This article is issued from Wikipedia - version of the Tuesday, March 22, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.