The launching of galactic winds from a multiphase ISM
Galactic outflows are a key agent of galaxy evolution, yet their observed multiphase nature remains difficult to reconcile with theoretical models, which often fail to explain how cold gas survives interactions with hot, fast winds. We present high-resolution three-dimensional hydrodynamic simulatio...
Enregistré dans:
| Auteurs principaux: | , , |
|---|---|
| Format: | Article (Journal) |
| Langue: | anglais |
| Publié: |
19 March 2026
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2026, Volume: 548, Numéro: 1, Pages: 1-21 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stag539 |
| Accès en ligne: | Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stag539 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/548/1/stag539/8529016 
|
| Notes sur l'auteur: | Fernando Hidalgo-Pineda, Max Gronke, Philipp Grete |
| Résumé: | Galactic outflows are a key agent of galaxy evolution, yet their observed multiphase nature remains difficult to reconcile with theoretical models, which often fail to explain how cold gas survives interactions with hot, fast winds. We present high-resolution three-dimensional hydrodynamic simulations of hot outflows interacting with a multiphase interstellar medium (ISM), parametrized by its cold-gas volume filling fraction [...] |
|---|---|
| Description: | Gesehen am 02.06.2026 Online veröffentlicht: 19. März 2026 |
| Description matérielle: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stag539 |