CP Puppis and V1500 Cygni

Details CP Puppis and V1500 Cygni CP Puppis and V1500 Cygni

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.217p...1w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 217, Nov. 1, 1985, p. 1P-5P.

Astronomy and Astrophysics

Astronomy

25

Astronomical Photometry, Novae, Periodic Variations, Stellar Activity, Amplitudes, Light Curve, Maxima

Scientific paper

Photometric observations of CP Puppis (Nova Puppis 1942) show recurrent humps with a period of 0.06614 day (or its 1-day alias 0.06196 day). The orbital light curve is very similar to that of V1500 Cyg (Nova Cygni 1975); both stars were very fast novae of exceptionally large amplitude. The photometric period of CP Puppis is significantly different from the recently reported spectroscopic period which may indicate a "superhump" or "intermediate polar" model for the system.

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