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Why Do Stars Turn Red? I. Post-Main-Sequence Expansion Mechanism

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Ou, Po-Sheng, Chen, Ke-Jung
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Solar and Stellar Astrophysics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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