THE EMISSION LINE SPECTRA OF CATACLYSMIC VARIABLE ACCRETION DISKS.
An explanation of the emission line behavior in cataclysmic variables has been among the most important and elusive problems in eruptive star research. This work expands accretion disk chromosphere models of line emission to predict line behavior qualitatively. A search for UX UMa-like thick disk ca...
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| Language: | en |
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The University of Arizona.
1983
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| Online Access: | http://hdl.handle.net/10150/187596 |