paper

The fate of central black holes in merging galaxies

arXiv:astro-ph/9407018 · doi:10.1093/mnras/271.2.317

Abstract

This paper presents results of a series of numerical N-body experiments that describe the merging of galaxy pairs containing a massive black hole in their core. The aim is to study the orbital evolution of the two black holes through the merger event. It is found that merging does NOT lead to the formation of a CLOSE black hole pair} at the center of the remnant when the two progenitor galaxies have (1) similar masses, (2) different central densities, and (3) relative orbit with non zero angular momentum. Under these conditions, the central black hole of the less dense galaxy settles into an wide orbit, i.e., at a distance from the center comparable to the half mass radius of the remnant, where the time scale for orbital decay by dynamical friction can be several Gyrs. The implications of this result are briefly discussed.

7 pages (4 figures included), uuencoded tared postscript file, accepted to the MNRAS, 1 additional figure available upon request from [email protected]

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