Analysis of the AAVSO light curves of 21 dwarf novae

Details Analysis of the AAVSO light curves of 21 dwarf novae Analysis of the AAVSO light curves of 21 dwarf novae

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..988s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Dec. 1984, p. 988-995.

Other

118

Dwarf Novae, Light Curve, Spectrum Analysis, Variable Stars, Orbital Elements, Stellar Mass

Scientific paper

The authors report the measurement of all observed outbursts of 21 dwarf novae during a three-year interval (JD2442300 - JD2443300), using the data records of the AAVSO. Relationships among the rise time, outburst length, decline time, quiescent interval, maximum V magnitude, and physical-system parameters such as orbital period and masses of the component stars were investigated. The results confirm some, but not all, of the correlations previously found for the best-studied system SS Cyg and other, less consistent, surveys. The autors use the long- and short-outburst separation characteristic of the SU UMa class to identify several prime suspects for this group.

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