Markarian 335
| Markarian 335 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 00h 06m 19.582s[1] |
| Declination | +20° 12′ 10.58″[1] |
| Redshift | 7730 km/s[2] |
| Heliocentric radial velocity | 0.025785[2] |
| Distance | 490.21 ± 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] | |
Markarian 335 is a Seyfert galaxy containing a supermassive black hole, located 324 million light-years away in the constellation of Pegasus.
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]
Gallery
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Graph showing the intensity vs. the energy (in keV) of X-rays coming from Markarian 335.
References
- ^ a b 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.
- ^ a b c "NED results for object MRK 0335". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 24 May 2018.
- ^ a b c d "Mrk 335". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 May 2018.
- ^ 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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