New light curves and analysis of the short-period Algol XZ Canis Minoris

Details New light curves and analysis of the short-period Algol XZ Canis Minoris New light curves and analysis of the short-period Algol XZ Canis Minoris

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..149t&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 106, no. 696, p. 149-153

Astronomy and Astrophysics

Astronomy

6

Binary Stars, Ephemerides, Light Curve, Stellar Radiation, Stellar Systems, Astronomical Photometry, Periodic Variations, Triple Stars

Scientific paper

We present new observations of the short-period Algol XZ Canis Minoris made between 25 Dec. 1992 and 1 Mar. 1993. Two new epochs of minimum light were determined and an improved ephemeris is given. Analysis of the observations with the latest version of the Wilson-Devinney program shows that the system is semidetached. Our solution does not indicate the presence of third light, whereas some previously published solutions required large amounts of third light.

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