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Close stellar binaries are prone to undergo a phase of stable mass transfer in which a star loses mass to its companion.
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2012
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C. A. Tout, Non-Conservative Evolution of Binary Stars, in From Interacting Binaries to Exoplanets: Essential Modeling Tools , Vol. 282, edited by M. T. Richards and I. Hubeny (2012) pp. 417–424
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K. Pavlovskii and N. Ivanova, Mass transfer from giant donors, MNRAS 449
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2016
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2016
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2016
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2017
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2018
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O. Tange, GNU Parallel 2018 (Ole Tange, 2018)
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2019
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2019
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2020
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