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Nuclear Spirals and Supermassive Black Holes

Published online by Cambridge University Press:  26 May 2016

H. B. Ann  and
Parijat Thakur
H. B. Ann
Affiliation:
Division of Science Education, Pus an National University, Busan 609735, Korea
Parijat Thakur
Affiliation:
Division of Science Education, Pus an National University, Busan 609735, Korea

Abstract

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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 speed in the gas.

Type
Part 9: Disks
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 315 - 316
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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