Recurrence behaviour of dwarf novae - The Kukarkin-Parenago relation

Details Recurrence behaviour of dwarf novae - The Kukarkin-Parenago relation Recurrence behaviour of dwarf novae - The Kukarkin-Parenago relation

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...144..199v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 144, no. 1, March 1985, p. 199-201.

Astronomy and Astrophysics

Astrophysics

13

Cataclysmic Variables, Dwarf Novae, Stellar Flares, Stellar Mass Accretion, Amplitudes, Correlation, Mass Transfer, Temporal Distribution

Scientific paper

The amplitudes and average recurrence times of dwarf novae are
correlated. The slope of the Kukarkin-Parenago relation suggests an
underlying regularity in the average dwarf-nova outburst behaviour which
may imply that on average the amount of matter transferred during
quiescence has an approximately constant value for all dwarf novae.

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