Structure of the super-Eddington outflow and its impact on the cosmological scale
Abstract It is one of the biggest issues in black hole (BH) astrophysics how to evaluate BH feedback to its environments precisely. Aiming at studying the unique gas dynamics of super-Eddington flow around supermassive black hole (SMBH) seeds at high redshift, we carried out axisymmetric two-dimensi...
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| Veröffentlicht in: | Publications of the Astronomical Society of Japan 2022-04, Vol.74 (2), p.384-397 |
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| Hauptverfasser: | , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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