Orbital elements of the exnova CP Puppis

Details Orbital elements of the exnova CP Puppis Orbital elements of the exnova CP Puppis

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.229..653d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 229, Dec. 15, 1987, p. 653-657.

Astronomy and Astrophysics

Astronomy

14

Binary Stars, Novae, Orbital Elements, Radial Velocity, Astronomical Photometry, Spectrum Analysis, Stellar Mass, Stellar Spectra

Scientific paper

Radial velocity measurements of the exnova CP Pup yield an orbital
amplitude of 92 km/s and a period of 0.0614215 day, which is shorter
than the photometric periods determined by Warner (1985). The mass of
the secondary is 0.14 solar mass; that of the primary is below 0.86
solar mass, perhaps as low as 0.12 solar mass.

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