Abstract
Pre-Main-Sequence contracting objects, post-Main-Sequence expanding stars and mass-losing components of semi-detached systems all occupy more or less the same region in the conventional H-R-diagram. We make a transformation to variables Δ (logL) and Δ (log T e), where Δ is the difference between the observed quantity, logL or log T e, and the value of that quantity which a star of the same mass would have on the empirical Main Sequence. It is demonstrated that a plot between the new variables clearly separates the mass-losing stars from other objects which is essentially an effect of the increasing abundance of helium relative to hydrogen.
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© 1984 D. Reidel Publishing Company, Dordrecht, Holland
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Abhyankar, K.D. (1984). Mass Loss in Semi-Detached Binaries. In: Hidayat, B., Kopal, Z., Rahe, J. (eds) Double Stars, Physical Properties and Generic Relations. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6372-6_35
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DOI: https://doi.org/10.1007/978-94-009-6372-6_35
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