The photometric variability of massive stars due to gravity waves excited by core convection

Massive stars die in catastrophic explosions that seed the interstellar medium with heavy elements and produce neutron stars and black holes. Predictions of the explosion’s character and the remnant mass depend on models of the star’s evolutionary history. Models of massive star interiors can be emp...

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Detalles Bibliográficos
Autores principales: Anders, Evan H., Lecoanet, Daniel, Cantiello, Matteo, Burns, Keaton J., Hyatt, Benjamin A., Kaufman, Emma, Townsend, Richard H. D., Brown, Benjamin P., Vasil, Geoffrey M., Oishi, Jeffrey S., Jermyn, Adam S.
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/PMC10581898/
https://www.ncbi.nlm.nih.gov/pubmed/37859938
http://dx.doi.org/10.1038/s41550-023-02040-7

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10581898/
https://www.ncbi.nlm.nih.gov/pubmed/37859938
http://dx.doi.org/10.1038/s41550-023-02040-7

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