No CrossRef data available.
Article contents
The Kukarkin-Parenago Relation for Dwarf Novae and Novae
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The period-amplitude relation and the period-energy relation for dwarf novae and novae are discussed. The total outbursts energy is shown to be a more suitable characteristic of the outburst than its amplitude.
- Type
- V. Nova and Dwarf Nova Outbursts
- Information
- Copyright
- Copyright © Reidel 1987
References
Holm, A.V., Wu, Chi-Chao, Sparks, W.M., Schiffer, F.H., Boggess, A., 1980. “Close Binary Stars: Observ. and Interpretat”. Dordrecht, e.a., 447.Google Scholar
Kukarkin, B.V., Kholopov, P.N., Efremov, Yu. N., Kukarkina, N.P., Kurochkin, N.E., Medvedeva, G.I., Perova, N.B., Fedorovich, V.P., Frolov, M.C.,1969. General Cataloque of Variable Stars. Moscow.Google Scholar
McDonald, J., 1983. “Cataclysmic. Var. and Relat. Objects”, 72 Colloq. Astron. Union. Haifa, 77.Google Scholar
Ortolani, S., Rafanelli, P., Rosino, L., Vittone, A., 1980. Astron. Astrophys., 87, 31.Google Scholar
Pskovskii, Yu.P., 1974. “Novae and Supernovae”, Moscow, ed. Science. Schmidt-Kaler Th., 1962. Kleine Veröff der Remeis-Sternwarte Bamberg, 34, 109.Google Scholar