Electromagnetic Counterparts Powered by Kicked Remnants of Black Hole Binary Mergers in AGN Disks

Electromagnetic Counterparts Powered by Kicked Remnants of Black Hole Binary Mergers in AGN Disks

The disk of an active galactic nucleus (AGN) is widely regarded as a prominent formation channel of binary black hole (BBH) mergers that can be detected through gravitational waves (GWs). Besides, the presence of dense environmental gas offers the potential for an embedded BBH merger to produce elec...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй
Үндсэн зохиолчид:	Ken Chen, Zi-Gao Dai
Формат:	Өгүүллэг
Хэл сонгох:	English
Хэвлэсэн:	IOP Publishing 2024-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Active galactic nuclei Accretion Black holes Gravitational wave sources Jets
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/ad0dfd

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