Unstable Mass Transfer from a Main-sequence Star to a Supermassive Black Hole and Quasiperiodic Eruptions
We discuss the formation and evolution of systems composed of a low-mass ( M _⋆ ≲ 4 M _⊙ ) main-sequence star orbiting a 10 ^5 –10 ^7 M _⊙ supermassive black hole with an orbital period of order ∼hours and a mild eccentricity ( e ≈ 0.1–0.2), episodically shedding mass at each pericenter passage. We...
Sábháilte in:
| Príomhchruthaitheoirí: | , |
|---|---|
| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe / Cruthaithe: |
IOP Publishing
2023-01-01
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| Sraith: | The Astrophysical Journal |
| Ábhair: | |
| Rochtain ar líne: | https://doi.org/10.3847/1538-4357/acbd3d |
| Clibeanna: |
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