Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-11-06
Astron.Astrophys. 411 (2003) 71-76
Astronomy and Astrophysics
Astrophysics
6 pages, 2 figures, accepted by Astronomy & Astrophysics
Scientific paper
10.1051/0004-6361:20031334
We present here a new determination of the ratio of energies radiated by active galactic nuclei and by stars and discuss the reasons for the apparently conflicting results found in previous studies. We conclude that the energy radiated by accretion processes onto super massive black holes is about 1 to 5% of the energy radiated by stars. We also estimate that the total mass accreted on average by a super massive black hole at the centre of a typical 10^11 Msol galaxy is of about 7 10^7 Msol.
Courvoisier Thierry J. -L.
Türler Marc
Zurita Heras Juan A.
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