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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| Hauptverfasser: | , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
IOP Publishing
2026-01-01
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| Schriftenreihe: | The Astrophysical Journal |
| Schlagworte: | |
| Online-Zugang: | https://doi.org/10.3847/1538-4357/ae3726 |
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