The Fate of Massive Black Holes in Gas-Rich Galaxy Mergers

Physics

Scientific paper

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Black Hole Physics, Cosmology: Theory, Galaxies: Evolution, Hydrodynamics, Quasars: General

Scientific paper

Using SPH numerical simulations, we investigate the effects of gas on the inspiral and merger of a massive black hole binary. This study is motivated by the very massive nuclear gas disks observed in the central regions of merging galaxies. Here we present results that expand on the treatment in previous works (Escala et al. 2004, 2005), by studying the evolution of a binary with different black holes masses in a massive gas disk.

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