The first stars: formation, properties, and impact
The first generation of stars, often called Population III (or Pop III), form from metal-free primordial gas at redshifts z ∼ 30 and below. They dominate the cosmic star-formation history until z ∼ 15–20, at which point the formation of metal-enriched Population II stars takes over. We review curren...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
August 2023
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| In: |
Annual review of astronomy and astrophysics
Year: 2023, Jahrgang: 61, Pages: 65-130 |
| ISSN: | 1545-4282 |
| DOI: | 10.1146/annurev-astro-071221-053453 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.1146/annurev-astro-071221-053453 Verlag, kostenfrei, Volltext: https://www.annualreviews.org/doi/10.1146/annurev-astro-071221-053453 
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| Verfasserangaben: | Ralf S. Klessen and Simon C.O. Glover |
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| 520 | |a The first generation of stars, often called Population III (or Pop III), form from metal-free primordial gas at redshifts z ∼ 30 and below. They dominate the cosmic star-formation history until z ∼ 15–20, at which point the formation of metal-enriched Population II stars takes over. We review current theoretical models for the formation, properties, and impact of Pop III stars and discuss existing and future observational constraints. ... | ||
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