Unstable Mass Transfer from a Main-Sequence Star to a Supermassive Black Hole and Quasi-Periodic Eru...
Unstable Mass Transfer from a Main-Sequence Star to a Supermassive Black Hole and Quasi-Periodic Eruptions
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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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We discuss the formation and evolution of systems comprised of a low-mass (\(M_\star \lesssim 4 \, \rm M_\odot\)) main sequence star, orbiting a \(10^5-10^7 \, \rm M_\odot\) supermassive black hole with an orbital period of order \(\sim\)hours, and a mild eccentricity (\(e\approx0.1-0.2\)), episodically shedding mass at each pericenter passage. We...
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Unstable Mass Transfer from a Main-Sequence Star to a Supermassive Black Hole and Quasi-Periodic Eruptions
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TN_cdi_proquest_journals_2738301746
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2738301746
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2211.09851
