A simple method to convert sink particles into stars
Hydrodynamical simulations of star formation often do not possess the dynamic range needed to fully resolve the build-up of individual stars and star clusters, and thus have to resort to sub-grid models. A popular way to do this is by introducing Lagrangian sink particles, which replace contracting...
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
10 December 2016
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 466, Heft: 1, Pages: 407-412 |
| ISSN: | 1365-2966 |
| Online-Zugang: |
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| Verfasserangaben: | Mattia C. Sormani, Robin G. Treß, Ralf S. Klessen and Simon C.O. Glover |
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A simple method to convert sink particles into stars
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