The orbital periodicity in the different outburst stages of Nova Cassiopeiae 1995 (V723 Cas)

Details The orbital periodicity in the different outburst stages of Nova Cassiopeiae 1995 (V723 Cas) The orbital periodicity in the different outburst stages of Nova Cassiopeiae 1995 (V723 Cas)

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..625g&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

The amplitude of the orbital periodicity with P = 0d.693265 changed from 0m.07 V in September 1997 to 0m.73 V in the second part of 2000. The system displays the properties of an eclipsing interacting binary. The small amplitude orbital light variations were found in the pre-maximum stage. The structure of system in outburst, and the nature of flaring episodes during the light decay are discussed.

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