An Illustration of Modeling Cataclysmic Variables: HST, FUSE, SDSS Spectra of SDSSJ080908.39+381406.2

作者: Albert P. Linnell , D. W. Hoard , Paula Szkody , Knox S. Long , Ivan Hubeny

DOI: 10.1086/507455

关键词: AstrophysicsSpectral lineAccretion discTomographic reconstructionCataclysmic variable starPhysicsFuse (electrical)

摘要: We use FUSE, HST, and SDSS spectra of the cataclysmic variable SDSSJ0809 to illustrate procedures for calculating testing system models. Our final model has an accretion disk temperature profile similar SW Sextantis determined from tomographic reconstruction.

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