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M82 X-1

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Suspected black hole
M82 X-1
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
SIMBADdata

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

  1. 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.
  2. 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.
  3. "Strange case of M82 X-1: A rare midsize black hole | EarthSky.org". earthsky.org. 19 August 2014. Retrieved 2019-03-03.

External links

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