UBVRI photometry of CP Puppis - A magnetic nova?

Details UBVRI photometry of CP Puppis - A magnetic nova? UBVRI photometry of CP Puppis - A magnetic nova?

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..964d&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Sept. 1991, p. 964-968.

Other

18

Cataclysmic Variables, Dwarf Novae, Magnetic Stars, Stellar Spectrophotometry, Ubv Spectra, White Dwarf Stars, Light Curve, Stellar Color, Stellar Luminosity, Stellar Magnetic Fields

Scientific paper

Results of about 16 hours of UBVRI photometry of Nova Pupis 1942 are presented. A modulation of the (B-V) color index with the 88-minute orbital period is found. This modulation is interpreted as a possible evidence for a strongly magnetized white dwarf in the system, and a comparison with other novae that are polars or intermediate polars is made.

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