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The imprint of star formation on stellar pulsations
In the earliest phases of their evolution, stars gain mass through the acquisition of matter from their birth clouds. The widely accepted classical concept of early stellar evolution neglects the details of this accretion phase and assumes the formation of stars with large initial radii that contrac...
Autores principales: | Steindl, Thomas, Zwintz, Konstanze, Vorobyov, Eduard |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2022
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9485136/ https://www.ncbi.nlm.nih.gov/pubmed/36123335 http://dx.doi.org/10.1038/s41467-022-32882-0 |
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