Propagation of a Precessing Jet in the Envelope of Tidal Disruption Events
It is likely that the disk of a tidal disruption event (TDE) is misaligned with respect to the equatorial plane of the spinning supermassive black hole (SMBH), since the initial stellar orbit before disruption most likely has an inclined orbital plane. Such a misaligned disk undergoes Lense–Thirring...
Wedi'i Gadw mewn:
| Prif Awduron: | , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
IOP Publishing
2025-01-01
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| Cyfres: | The Astrophysical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/ae1eed |
| Tagiau: |
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