Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
Aims. It is difficult to implement numerical simulations on a region extending from the vicinity of a black hole to the Bondi radius. Most previous numerical simulations have primarily concentrated on the region close to the black hole. They found that strong winds can be generated in the hot accret...
Uloženo v:
| Hlavní autoři: | , , |
|---|---|
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
EDP Sciences
2026-05-01
|
| Edice: | Astronomy & Astrophysics |
| Témata: | |
| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/05/aa57811-25/aa57811-25.html |
| Tagy: |
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
|