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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Podrobná bibliografie

Hlavní autoři:	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
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2026-06-01
Edice:	Astronomy & Astrophysics
Témata:	gravitational waves binaries: close stars: black holes stars: massive
On-line přístup:	https://www.aanda.org/articles/aa/full_html/2026/06/aa59298-26/aa59298-26.html
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