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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Detalhes bibliográficos

Principais autores:	Klencki Jakub, Podsiadlowski Philipp, Langer Norbert, Olejak Aleksandra, Justham Stephen, Vigna-Gómez Alejandro, de Mink Selma E.
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-02-01
Colecção:	Astronomy & Astrophysics
Assuntos:	gravitational waves binaries: general stars: black holes stars: evolution stars: interiors stars: massive
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/02/aa55500-25/aa55500-25.html
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