The Role of the Third Dredge-up and Mass Loss in Shaping the Initial–Final Mass Relation of White Dwarfs

The Role of the Third Dredge-up and Mass Loss in Shaping the Initial–Final Mass Relation of White Dwarfs

The initial–final mass relation (IFMR) plays a crucial role in understanding stellar structure and evolution by linking a star’s initial mass to the mass of the resulting white dwarf. This study explores the IFMR in the initial mass range 0.8 ≤ M _ini / M _⊙ ≤ 4 using full PARSEC evolutionary calcul...

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Autori principali: Francesco Addari, Paola Marigo, Alessandro Bressan, Guglielmo Costa, Kendall Shepherd, Guglielmo Volpato
Natura: Articolo
Lingua:English
Pubblicazione: IOP Publishing 2024-01-01
Serie:The Astrophysical Journal
Soggetti:
Asymptotic giant branch stars
Carbon stars
White dwarf stars
Stellar winds
Stellar convective zones
Accesso online:https://doi.org/10.3847/1538-4357/ad2067

Accesso online

https://doi.org/10.3847/1538-4357/ad2067

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