On the relevance of bubbles and potential flows for stellar convection
Recently Pasetto et al. have proposed a new method to derive a convection theory appropriate for the implementation in stellar evolution codes. Their approach is based on the simple physical picture of spherical bubbles moving within a potential flow in dynamically unstable regions, and a detailed c...
Guardado en:
| Autores principales: | Miller Bertolami, Marcelo Miguel, Viallet, Maxime, Prat, Vincent, Barsukow, Wasilij, Weiss, Achim |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93771 https://academic.oup.com/mnras/article/457/4/4441/2588982 https://ri.conicet.gov.ar/handle/11336/35721 |
| Aporte de: |
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