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Emission Lines of Dwarf Novae Accretion Disks

Published online by Cambridge University Press:  12 April 2016

W. Hummel ,
K. Horne ,
T. Marsh  and
J. H. Wood
W. Hummel
Affiliation:
Uni-Sternwarte München, Scheinerstr. 1, D–81679 München, Germany
K. Horne
Affiliation:
University of St. Andrews, School of Physics & Astronomy, North Haugh, St. Andrews, Fife, KY16 9SS, Scotland, UK
T. Marsh
Affiliation:
University of Southampton, Department of Physics, Highfield, Southampton SO17 1B J, England, UK
J. H. Wood
Affiliation:
Keele University, Department of Physics, Keele ST5 5BG, England, UK

Abstract

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We derive the temperature and density structure of the accretion disk of the dwarf nova U Gem in quiescence from 3D radiative line and continuum transport calculations of a differentially rotating disk.

Type
Part 10. Accretion Disks and Outflows
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 498 - 501
Copyright
Copyright © Astronomical Society of the Pacific 1997

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