Abstract
Almost exactly 40 years ago, quasars were discovered by M. Schmidt [43] and others. Soon thereafter, Zel’dovich [50] and Salpeter [42] suspected that accretion onto compact objects, like black holes, provided the only efficient and plausible way to generate the required luminosities. Little later, Lynden-Bell [28] refined the picture which became to be known as the black hole paradigm for active galactic nuclei.
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Bender, R. Supermassive Black Holes in Nearby Galaxy Centers. In: Merloni, A., Nayakshin, S., Sunyaev, R.A. (eds) Growing Black Holes: Accretion in a Cosmological Context. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/11403913_25
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DOI: https://doi.org/10.1007/11403913_25
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