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The spectroscopic period of the cataclysmic system AM CVn

✍ Scribed by C. Lázaro; J. E. Solheim; M. J. Arévalo

Publisher: Springer Netherlands
Year: 1990
Tongue: English
Weight: 97 KB
Volume: 169
Category: Article
ISSN: 0004-640X
DOI: 10.1007/bf00640729

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## Abstract We briefly summarise the observational properties of ultra‐compact binaries called AM CVn stars. We analyse their outbursts originating from the thermal‐viscous instability in helium accretion disc. We present our preliminary results in applying the model of Dwarf Novae outbursts to hel