Markarian 335

Markarian 335 is a Seyfert galaxy containing a supermassive black hole, located 324 million light-years away in the constellation of Pegasus.

Markarian 335
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension00h 06m 19.582s[1]
Declination+20° 12 10.58[1]
Redshift7730 km/s[2]
Helio radial velocity0.025785[2]
Distance490.21 ± 217.40 Mly (150.300 ± 66.654 Mpc)[2]
Apparent magnitude (V)13.85[3]
Apparent magnitude (B)14.19[3]
Characteristics
Apparent size (V)0.187′[3]
Other designations
INTREF 2, 2MASS J00061953+2012105, PGC 473[3]

The central black hole in this active galaxy nucleus is notable for its corona's spinning rate (at about 20 percent the speed of light) and its change in brightness from 2007 to 2014. The geometry of the corona has been deduced from relativistic blurring of the reflection of the accretion disc. An x-ray flare in 2013 is interpreted as an aborted jet.[4]

References

  1. Skrutskie, M.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
  2. "NED results for object MRK 0335". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 24 May 2018.
  3. "Mrk 335". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 May 2018.
  4. Wilkins, D. R; Gallo, L. C (2015). "Driving extreme variability: The evolving corona and evidence for jet launching in Markarian 335". Monthly Notices of the Royal Astronomical Society. 449: 129. arXiv:1501.05302. Bibcode:2015MNRAS.449..129W. doi:10.1093/mnras/stv162.
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