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• W3098481623 endingPage "672" @default.
• W3098481623 startingPage "655" @default.
• W3098481623 abstract "We present a study of the secular evolution of a spherical stellar system with a central star-accreting black hole (BH) using the anisotropic gaseous model. This method solves numerically moment equations of the full Fokker–Planck equation, with Boltzmann–Vlasov terms on the left-hand side and collisional terms on the right-hand side. We study the growth of the central BH due to star accretion at its tidal radius and the feedback of this process on to the core collapse as well as the post-collapse evolution of the surrounding stellar cluster in a self-consistent manner. Diffusion in velocity space into the loss cone is approximated by a simple model. The results show that the self-regulated growth of the BH reaches a certain fraction of the total mass cluster and agrees with other methods. Our approach is much faster than competing ones (Monte Carlo, N-body) and provides detailed information about the time- and space-dependent evolution of all relevant properties of the system. In this paper we present the method and study simple models (equal stellar masses, no stellar evolution or collisions). None the less, a generalization to include such effects is conceptually simple and under way." @default.
• W3098481623 created "2020-11-23" @default.
• W3098481623 creator A5022615067 @default.
• W3098481623 creator A5043636886 @default.
• W3098481623 creator A5045375802 @default.
• W3098481623 date "2004-08-01" @default.
• W3098481623 modified "2023-10-01" @default.
• W3098481623 title "Accretion of stars on to a massive black hole: a realistic diffusion model and numerical studies" @default.
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• W3098481623 doi "https://doi.org/10.1111/j.1365-2966.2004.07956.x" @default.
• W3098481623 hasPublicationYear "2004" @default.
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