Interacting Binaries on the Main Sequence as In Situ Tracers of Mass-transfer Efficiency and Stability

Understanding the transfer of mass and angular momentum in binary interactions is crucial for modeling the evolution of any interacting binary after the first mass-transfer phase. Mass-transfer physics assumptions shape the predictions for later stages of binary evolution, such as the immediate prog...

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Hlavní autoři:	Koushik Sen, Mathieu Renzo, Harim Jin, Norbert Langer, Abel Schootemeijer, Jaime I. Villaseñor, Laurent Mahy, Aldana Grichener, Neev Shah, Chen Wang, Xiao-Tian Xu
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	Algol variable stars Eclipsing binary stars Stellar evolution Stellar interiors
On-line přístup:	https://doi.org/10.3847/1538-4357/ae40fc
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