Markarian 709

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Mrk 709
2MASS image of the pair of galaxies Mrk 709
2MASS image (former JHK composite, incorrectly converted to grayscale)
Observation
dates equinoxJ2000.0
Constellation lion
Right ascension 9491809 h 49 m 18 s
declination 2165270+ 16 ° 52.7 ′ 0 ″
Physical data
Redshift approx. 0.052
distance approx. 210 M pc
approx. 700 M ly
Designations and catalog entries
PGC  28237 • IRAS F09466 + 1706 • 2MASX J09491806 + 1652448

Mrk 709 ( Markarian 709 ) is a pair of two low- metallicity dwarf galaxies that are believed to interact with each other. Due to the redshift of this system consisting of the components Mrk 709 S and Mrk 709 N of z = 0.052, a distance of around 200 million parsecs (around 700 million light years) can be assumed. In Mrk 709 S, Reines et al. Evidence of an active supermassive black hole found; they estimated the stellar masses of the galaxies to be around 2.5 billion solar masses for Mrk 709 S and 1.1 billion solar masses for Mrk 709 N. With 10% of solar metallicity, Mrk 709 is one of the most metal-poor galaxies showing signs of an active galaxy core.

swell

  • Reines et al .: A candidate massive black hole in the low-metallicity dwarf galaxy pair Mrk 709 ; The Astrophysical Journal Letters 787 (2), 2014, bibcode : 2014ApJ ... 787L..30R

Individual evidence

  1. a b NED