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Emission Lines of Dwarf Novae Accretion Disks
Published online by Cambridge University Press: 12 April 2016
Abstract
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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