作者: Albert P. Linnell , D. W. Hoard , Paula Szkody , Knox S. Long , Ivan Hubeny
DOI: 10.1086/507455
关键词: Astrophysics 、 Spectral line 、 Accretion disc 、 Tomographic reconstruction 、 Cataclysmic variable star 、 Physics 、 Fuse (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.