Photometric Observations and Light Curve Studies of the Semi-Detached Eclipsing Binary R CMa |
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Authors: | M T Mirtorabi N Riazi |
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Institution: | (1) Physics Department, Azzahra University, Vanak, Tehran, Iran;(2) Physics Department and Biruni Observatory, Shiraz University, Shiraz, 71457, Iran |
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Abstract: | We present observations and light curve analysis of the eclipsing binary R CMa in the narrow band filters v and b. Observations were made during 1993 at Biruni Observatory and the light curves have been analyzed using the Wilson-Devinney
light curve interpretation program. Assuming a semi-detached configuration for R CMa, the parameters i, Ω1, L
1, T
2 and A
2 were adjusted for the best fit between the synthesized light curves and observations. Both light curves were fitted well
with a lower value of bolometric albedo than what would be expected for a normal cool star with a convective envelope. The
masses of the primary and secondary components and the absolute dimensions of the stars have been calculated using the derived
relative dimensions from Wilson-Devinney codes and the spectroscopic observations. |
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Keywords: | Stars: eclipsing binaries Stars: individual Stars: fundamental parameters |
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