Dynamic Disk–Corona Coupling during the State Transition of Swift J1727.8–1613

State transitions during outbursts of black hole X-ray binaries (BHXBs) exhibit complex, rapidly evolving disk–corona coupling. Understanding this dynamic phase is essential for deciphering accretion physics and the mechanisms that drive outbursts, yet it remains poorly understood because of the sca...

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Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	Han He, Yi Long, Bei You, Fu-Guo Xie, Zhen Yan, Andrzej A. Zdziarski, Sai-En Xu
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2026-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Low-mass x-ray binary stars Accretion X-ray binary stars Black holes High energy astrophysics
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/ae8094
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!