Light Curve and Analysis of the Eclipsing Binary BF Centauri

Details Light Curve and Analysis of the Eclipsing Binary BF Centauri Light Curve and Analysis of the Eclipsing Binary BF Centauri

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20314806m&link_type=abstract

American Astronomical Society Meeting 203, #148.06; Bulletin of the American Astronomical Society, Vol. 36, p.594

Astronomy and Astrophysics

Astronomy

Scientific paper

The eclipsing binary star BF Centauri was observed photometrically by GWW in the uvby filter system from Mt. John Observatory in New Zealand during 1982, 1989 and 1998. It was also observed spectroscopically at 10 A/mm by W. A. Lawson in 1993 at Mt. Stromlo in Australia to obtain a radial velocity solution. The combined light curves and spectroscopic results have been analyzed using the 1998 version of Robert Wilson's WD light-curve programs. A consistent model for the system will be presented. This analysis was done as a part of a senior research project by MAM, who would like to acknowledge financial support from the Missouri Space Grant Consortium.

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