Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Ursa Major |
Right ascension | 09 55 50.01 |
Declination | 69° 40′ 46.0″ |
Database references | |
SIMBAD | data |
M82 X-1 is an ultra-luminous X-ray source located in the galaxy M82. It is a candidate intermediate-mass black hole, with the exact mass estimate varying from around 100 to 1000 solar masses. One of the most luminous ULXs ever known, its luminosity exceeds the Eddington limit for a stellar mass object.
See also
References
- Fiorito, Ralph; Titarchuk, Lev (2004). "Is M82 X-1 Really an Intermediate-Mass Black Hole? X-Ray Spectral and Timing Evidence". The Astrophysical Journal. 614 (2): L113 – L116. arXiv:astro-ph/0409416. Bibcode:2004ApJ...614L.113F. doi:10.1086/425736. S2CID 10183683.
- Brightman, Murray; Harrison, Fiona A.; Barret, Didier; Davis, Shane W.; Fürst, Felix; Madsen, Kristin K.; Middleton, Matthew; Miller, Jon M.; Stern, Daniel; Tao, Lian; Walton, Dominic J. (2016). "A Broadband X-Ray Spectral Study of the Intermediate-mass Black Hole Candidate M82 X-1 with NuSTAR, Chandra, and Swift". The Astrophysical Journal. 829 (1): 28. arXiv:1607.03903. Bibcode:2016ApJ...829...28B. doi:10.3847/0004-637X/829/1/28. S2CID 19765183.
- "Strange case of M82 X-1: A rare midsize black hole | EarthSky.org". earthsky.org. 19 August 2014. Retrieved 2019-03-03.
External links
- Dying Star Reveals More Evidence for New Kind of Black Hole Archived 2021-11-20 at the Wayback Machine
- A medium-sized black hole? Archived 2010-01-13 at the Wayback Machine
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