Comfort zones of stars: A limit on orbital tightening via stable mass transfer shapes the properties of binary black hole mergers
Mass transfer in binary systems is the key process in the formation of various classes of objects, including merging binary black holes (BBHs) and neutron stars. The orbital evolution that occurs during mass transfer depends on how much mass is accreted and how much angular momentum is lost – two of...
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| Hlavní autoři: | , , , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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EDP Sciences
2026-02-01
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| Edice: | Astronomy & Astrophysics |
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| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/02/aa55500-25/aa55500-25.html |
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