Migration of supermassive black holes in galactic nuclei

Details Migration of supermassive black holes in galactic nuclei Migration of supermassive black holes in galactic nuclei

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008astl...34..537k&link_type=abstract

Astronomy Letters, Volume 34, Issue 8, pp.537-541

Astronomy and Astrophysics

Astronomy

Scientific paper

The migration of central black holes in galactic nuclei through their encounters with galactic globular clusters is studied. The black hole moves in the field of the galactic bulge with a fixed potential. The dependences of the black-hole drift amplitude on orbital parameters of the globular cluster, its mass, and bulge parameters have been found. The drift amplitude of the central black hole can reach several parsecs in our Galaxy and several tens of parsecs in early-type (Sa) and late-type (Sc) spiral galaxies.

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