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A metal-poor star with abundances from a pair-instability supernova
The most massive and shortest-lived stars dominate the chemical evolution of the pre-galactic era. On the basis of numerical simulations, it has long been speculated that the mass of such first-generation stars was up to several hundred solar masses(1–4). The very massive first-generation stars with...
| Autores principales: | , , , , , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2023
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10284693/ https://www.ncbi.nlm.nih.gov/pubmed/37286602 http://dx.doi.org/10.1038/s41586-023-06028-1 |