Long-term (250 yr) Hydrodynamical Simulation of the Supermassive Black Hole Binary OJ 287

With upcoming facilities capable of detecting photometric and gravitational wave signals from supermassive black hole (SMBH) binaries, studying their long-term accretion-driven variability is timely. OJ 287 is a bright, nearby ( z = 0.3), and well-studied candidate for an SMBH binary. As such, it is...

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Detalles Bibliográficos

Principais autores:	Ariel Chitan, Sarah C. Gallagher, Shahram Abbassi
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2026-01-01
Series:	The Astrophysical Journal
Assuntos:	Black holes Blazars Active galactic nuclei Accretion Hydrodynamical simulations Gravitational wave sources
Acceso en liña:	https://doi.org/10.3847/1538-4357/ae3726
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