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A Spectrum Synthesis and Light Synthesis Program for Binary Stars with Optically Thick Accretion Disks

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A. P. Linnel1,3 and I. Hubeny2,4

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[1]

The Reflection Effect in Interacting Binaries or in Planet-Star Systems

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A Method for the Study of Accretion Disk Emission in Cataclysmic Variables. I. The Model

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Synthetic Spectrum Constraints on a Model of the Cataclysmic Variable QU Carinae

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Albert P. Linnell et al.  The Astrophysical Journal 2007  662 1204
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[12]

An Illustration of Modeling Cataclysmic Variables: HST, FUSE, and SDSS Spectra of SDSS J080908.39+381406.2

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[13]

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[16]

The Hot White Dwarf in the Cataclysmic Variable MV Lyrae

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Resonance Line Profile Calculations Based on Hydrodynamical Models of Cataclysmic Variable Winds

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[19]

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[20]

RXTE, ROSAT, EUVE, IUE, and Optical Observations through the 45 Day Supercycle of V1159 Orionis

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[21]

New Light Synthesis and Spectrum Synthesis Constraints on a Model for β Lyrae

A. P. Linnell et al.  The Astrophysical Journal 1998  509 379
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