A case for Case A: Detailed look at binary black hole formation through stable mass transfer

Context. In isolated binary evolution, binary black hole (BBH) mergers are generally formed through stable mass transfer (SMT) or common envelope evolution. In recent years, the SMT channel has received significant attention due to detailed binary models showing increased mass transfer stability com...

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Autors principals:	Briel Max M., Fragos Tassos, Gallegos-Garcia Monica, Ray Anarya, Zevin Michael, Chattaraj Abhishek, Andrews Jeff J., Kalogera Vicky, Gossage Seth, Srivastava Philipp M., Teng Elizabeth
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-06-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	gravitational waves binaries: close stars: black holes stars: massive
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/06/aa59298-26/aa59298-26.html
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