Radial Pulsation of the Cooling White Dwarf in the Decay of Nova Cassiopeiae 1995 (V723 Cas)

Details Radial Pulsation of the Cooling White Dwarf in the Decay of Nova Cassiopeiae 1995 (V723 Cas) Radial Pulsation of the Cooling White Dwarf in the Decay of Nova Cassiopeiae 1995 (V723 Cas)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..311g&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3

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Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Pulsations, Oscillations, And Stellar Seismology

Scientific paper

The episode of oscillations with the period of 90m was observed on September 19, 1999 in the light decay stage of V723 Cas. This is a slow nova having highly inclined orbit with the period of 0.693265 days. The phenomenon is explained by pulsations in the expanded envelope of white dwarf. The possibility of pulsations was earlier predicted by K. Schenker.

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