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Supermassive black holes: Relation to dark halos

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Abstract

Estimates of the masses of supermassive black holes (M bh ) in the nuclei of disk galaxies with known rotation curves are compared with estimates of the rotational velocities V m and the “indicative” masses of the galaxies M i . Although there is a correlation between M bh and V m or M i , it is appreciably weaker than the correlation with the central velocity dispersion. The values of M bh for early-type galaxies (S0-Sab), which have more massive bulges, are, on average, higher than the values for late-type galaxies with the same rotational velocities. We conclude that the black-hole masses are determined primarily by the properties of the bulge and not the rotational velocity or the mass of the galaxy.

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992, Russia

    A. V. Zasov, L. N. Petrochenko & A. M. Cherepashchuk

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  1. A. V. Zasov
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  2. L. N. Petrochenko
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  3. A. M. Cherepashchuk
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__________

Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 82, No. 5, 2005, pp. 407–413.

Original Russian Text Copyright © 2005 by Zasov, Petrochenko, Cherepashchuk.

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Zasov, A.V., Petrochenko, L.N. & Cherepashchuk, A.M. Supermassive black holes: Relation to dark halos. Astron. Rep. 49, 362–367 (2005). https://doi.org/10.1134/1.1923545

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