A new approach to determine optically thick H2 cooling and its effect on primordial star formation
Gespeichert in:
| Weitere Verfasser: | , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
2014
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| In: |
Arxiv
Year: 2014, Pages: ? |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1407.2102
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| Verfasserangaben: | Tilman Hartwig; Paul C. Clark; Simon C. O. Glover; Ralf S. Klessen; Mei Sasaki |
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