CCD Photometry of Low Mass Ratio Contact Binary FP Boo - IV

Details CCD Photometry of Low Mass Ratio Contact Binary FP Boo - IV CCD Photometry of Low Mass Ratio Contact Binary FP Boo - IV

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jass...26....1o&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 26, no. 1, 1- 8

Astronomy and Astrophysics

Astronomy

1

Low Mass Ratio Contact Binary, Binary Solution, Evolution Of Binary Stars

Scientific paper

We present new B, V, and R CCD photometric light curves for the low mass ratio contact binay FP Boo. A new photometric solution and absolute physical dimensions of the system were derived by applying the Wilson-Devinney program to our observed light curves and to previously published Rucinski et al.'s radial velocity curves. From the H-R diagram of 24 low mass ratio contact binary system including FP Boo, the evolutionary stage of FP Boo was found to coincide with those of the general low mass ratio contact binary systems. The light curves obtained in this season show a small asymmetry in their shapes.

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