Nova remnants

Details Nova remnants Nova remnants

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236....1w&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 1-6 (SEE N86-20287 10-93)

Physics

7

Cataclysmic Variables, Novae, Stellar Evolution, Light Curve, Periodic Variations, Stellar Luminosity

Scientific paper

The brightest nova remnants and nova-like variables (which are possible candidates for membership of the class of nova remnants) are reviewed. Several nova remnants show multiple periodicities: V603 Aql, HR Del, CP Pup and possibly V1500 Cyg have differing photometric and spectroscopic periods. The cause of this is not known, but there is a similarity with the superhump phenomenon in SU UMa stars. The RR Pic shows changes in structure, 50 yr after the outburst.

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