Nuclear Spirals and Supermassive Black Holes
Astrophysics
2007-05-23 v1
Abstract
We have performed SPH simulations for the response of the gaseous disks to the imposed potentials including those from bars and SMBHs. Evolution of the nuclear regions of gaseous disks depends critically on the masses of SMBHs as well as the sound speeds in the gas.
Keywords
Cite
@article{arxiv.astro-ph/0408326,
title = {Nuclear Spirals and Supermassive Black Holes},
author = {H. B. Ann and Parijat Thakur},
journal= {arXiv preprint arXiv:astro-ph/0408326},
year = {2007}
}
Comments
2 pages, 1 Postscript figures, appeared in International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano, M. A. Walker, and K. C. Freeman. San Francisco: Astronomical Society of the Pacific