Dwarf Novae with Newly Determined Parallaxes: Model Analyses of VY Aquarii, RU Pegasi, and T Leonis

Using newly determined parallaxes for dwarf novae, we have derived outburst accretion rates for VY Aqr, RU Peg, and T Leo, and for T Leo during quiescence. The two short‐period dwarf novae, VY Aqr and T Leo, show good agreement with optically thick steady‐state accretion disks in outburst, whereas R...

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Veröffentlicht in:	Publications of the Astronomical Society of the Pacific 2004-10, Vol.116 (824), p.926-930
Hauptverfasser:	Hamilton, R. T., Sion, E. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Accretion disks Dwarf novae Light curves Mass spectroscopy Optical bursts Photospheres Spectroscopic analysis Visible spectrum White dwarfs
Online-Zugang:	Volltext
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