Radiation-magnetohydrodynamic Simulations of Accretion Flow Formation After a Tidal Disruption Event
We perform 3D radiation-magnetohydrodynamic simulations of the evolution of the fallback debris after a tidal disruption event (TDE). We focus on studying the effects of magnetic fields on the formation and early evolution of the accretion flow. We find that large magnetic fields can increase the de...
Sábháilte in:
| Príomhchruthaitheoirí: | , , , |
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| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe / Cruthaithe: |
IOP Publishing
2025-01-01
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| Sraith: | The Astrophysical Journal |
| Ábhair: | |
| Rochtain ar líne: | https://doi.org/10.3847/1538-4357/ae044c |
| Clibeanna: |
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