A Limit Cycle Model For Long‐Term Optical Variations of V Sagittae: The Second Example of Accretion Wind Evolution
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/598/i=1/a=527/pdf
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1. A New Orbital Ephemeris and Reinterpretation of Spectroscopic Data for the Supersoft X-Ray Binary RX J0513.9−6951
2. The Large Magellanic Cloud Supersoft X-Ray Binary RX J0513.9-6951
3. Time‐resolved Spectroscopy of V Sagittae
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