Exploring the borderline between stable mass transfer and mergers in close binary evolution
Exploring the borderline between stable mass transfer and mergers in close binary evolution
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The majority of massive stars reside in binary systems, which are expected to experience mass transfer during their evolution. However, so far the conditions under which mass transfer leads to a common envelope, and thus possibly to a merging of both stars, are not well understood. Main uncertainties arise from the possible swelling of the mass gai...
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Exploring the borderline between stable mass transfer and mergers in close binary evolution
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TN_cdi_proquest_journals_3039010348
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3039010348
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2404.08615