Secular evolution and a non-evolving black hole to galaxy mass ratio in the last 7 Gyr

Details Secular evolution and a non-evolving black hole to galaxy mass ratio in the last 7 Gyr Secular evolution and a non-evolving black hole to galaxy mass ratio in the last 7 Gyr

2011-09-21

arxiv.org/abs/1109.4633v1

Astrophys.J.741:L11,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

7 pages, 4 figures, accepted for publication in ApJ Letters

Scientific paper

10.1088/2041-8205/741/1/L11

We present new constraints on the ratio of black hole (BH) mass to total galaxy stellar mass at 0.3

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