Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-26T20:38:38.831Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Adam, J. 1990, A&A 240, 541 Google Scholar
Friend, M.T., Martin, J.S., Smith, R.C., Jones, D.H.P. 1990, MNRAS 246, 637 Google Scholar
Hummel, W. 1994, A&A 289, 458 Google Scholar
Panek, R.J., Holm, A.V. 1984, ApJ 277, 700 Google Scholar
Press, W.H., Teuholsky, S.A., Vetterling, W.T., Flannery, B.P. 1992 Numerical Recipes in C, 2nd Ed., Cambridge University Press Google Scholar
Zhang, E.H., Robinson, E.L., 1987, ApJ 321, 813 CrossRefGoogle Scholar