NGC 4395

NGC 4395 is a low surface brightness spiral galaxy with a halo that is about 8 in diameter. It has several wide areas of greater brightness running northwest to southeast. The one furthest southeast is the brightest. Three of the patches have their own NGC numbers: 4401, 4400, and 4399 running east to west.[3] The nucleus of NGC 4395 is active and the galaxy is classified as a Seyfert. It is notable for containing one of the smallest supermassive black hole with an accurately-determined mass.[4] The central black hole has a mass of "only" 300,000 Sun masses,[5] which would make it a so-called "intermediate-mass black hole".

NGC 4395
An ultraviolet image of NGC 4395 taken with GALEX.
Credit: GALEX/NASA
Observation data (J2000 epoch)
ConstellationCanes Venatici[1]
Right ascension 12h 25m 48.9s[2]
Declination+33° 32 48[2]
Redshift319 ± 1 km/s[2]
Distance~14 million light-years
Apparent magnitude (V)10.6[2]
Characteristics
TypeSA(s)m[2]
Size50,000 ly (diameter)
Apparent size (V)13.2 × 11.0[2]
Other designations
NGC 4395,[3] UGC 7542,[2] PGC 40596[2]
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gollark: Bees will be caused to rotate as an inevitable consequence.
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gollark: ±39% error margin.
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References

  1. Celestia version 1.4.1. Laurel, Chris, 2006.
  2. "NASA/IPAC Extragalactic Database". Results for. Retrieved 2006-11-04.
  3. Kepple, George Robert; Glen W. Sanner (1998). The Night Sky Observer's Guide, Volume 2. Willmann-Bell, Inc. p. 48. ISBN 978-0-943396-60-6.
  4. Merritt, David (2013). Dynamics and Evolution of Galactic Nuclei. Princeton, NJ: Princeton University Press. ISBN 9781400846122.
  5. Peterson, Bradley; et al. (2005). "Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. I. A Reverberation-based Measurement of the Black Hole Mass". The Astrophysical Journal. 632 (2): 799–808. arXiv:astro-ph/0506665. Bibcode:2005ApJ...632..799P. doi:10.1086/444494.


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