A new approach to determine optically thick H2 cooling and its effect on primordial star formation
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| Other Authors: | , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2015
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| In: |
The astrophysical journal
Year: 2015, Volume: 799, Issue: 2, Pages: 114 |
| ISSN: | 1538-4357 |
| DOI: | 10.1088/0004-637X/799/2/114 |
| Online Access: | Verlag, kostenfrei, Volltext: http://iopscience.iop.org/0004-637X/799/2/114/ Resolving-System, kostenfrei, Volltext: http://dx.doi.org/10.1088/0004-637X/799/2/114 
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| Author Notes: | Tilman Hartwig; Paul C. Clark; Simon C. O. Glover; Ralf S. Klessen; Mei Sasaki |
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A new approach to determine optically thick H2 cooling and its effect on primordial star formation
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