Nuclear Spirals and Supermassive Black Holes

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dc.creatorAnn, H. B.
dc.creatorThakur, Parijat
dc.date2004-08-18
dc.date.accessioned2026-07-07T02:14:19Z
dc.date.available2026-07-07T02:14:19Z
dc.descriptionWe 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.
dc.description2 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0408326
dc.identifierhttp://arxiv.org/abs/astro-ph/0408326
dc.identifierIAUS 220 (2004) 315
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8069
dc.subjectAstrophysics
dc.titleNuclear Spirals and Supermassive Black Holes
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