Abstract
The dependence of mass ratio of eclipsing binary systems on period has been studied. It has been found that semi-detached systems obey the relationm 2/m 1=0.64–0.079P orm 2/m 1=0.29–0.028P depending upon whether the mass ratio is >0.3 or <0.3. The mass ratio of deteched systems generally appears to be independent of the period.
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Sinvhal, S.D., Srivastava, J.B. Period-mass ratio relations for eclipsing binaries with periods not exceeding 5 days. Astrophys Space Sci 54, 239–245 (1978). https://doi.org/10.1007/BF00637911
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DOI: https://doi.org/10.1007/BF00637911