Synthetic analysis of light curves of the close binary system UZ Puppis

Details Synthetic analysis of light curves of the close binary system UZ Puppis Synthetic analysis of light curves of the close binary system UZ Puppis

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..269m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 269-272.

Astronomy and Astrophysics

Astrophysics

3

A Stars, Binary Stars, Light Curve, Maxima, Roche Limit, Stellar Luminosity, Stellar Mass

Scientific paper

BV light curves obtained by Bookmyer (1985) have been analyzed with Yamasaki's synthetic technique. As some small difference exists between the light maxima, analysis has been made for the first and the second half of light curve, separately. The result indicates that system parameters deduced from the second half give a better fitting with smaller O-C residuals. These parameters reveal that UZ Pup is contact to the Roche lobe.

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