The very low state of V794 Aquilae

Details The very low state of V794 Aquilae The very low state of V794 Aquilae

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97.1189h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Dec. 1985, p. 1189-1191.

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8

Accretion Disks, Balmer Series, Cataclysmic Variables, Eclipsing Binary Stars, Stellar Mass Accretion, Stellar Spectrophotometry, Novae

Scientific paper

The cataclysmic variable V794 Aql was found to have dropped from its normal magnitude range of B ≈ 14 - 17 to B ≈ 20. In this very low state the accretion-disk emission lines were replaced by very narrow Balmer emission. This behavior is very similar to that of MV Lyr and a few other systems in which the accretion apparently switches off for brief periods of time.

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