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...

Descripción completa

Detalles Bibliográficos
Autores principales: Xing, Qian-Fan, Zhao, Gang, Liu, Zheng-Wei, Heger, Alexander, Han, Zhan-Wen, Aoki, Wako, Chen, Yu-Qin, Ishigaki, Miho N., Li, Hai-Ning, Zhao, Jing-Kun
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
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

Internet

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

Ejemplares similares