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Stellar Evolution in Real Time. II. R Hydrae and an Open-Source Grid of >3000 Seismic TP-AGB Models Computed with MESA

We present a comprehensive characterization of the evolved thermally pulsing asymptotic giant branch (TP-AGB) star R Hydrae (R Hya), building on the techniques applied in Stellar Evolution in Real Time I (Molnár et al.) to T Ursae Minoris. We compute over 3000 theoretical TP-AGB pulse spectra using...

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Auteurs principaux: Meridith Joyce, László Molnár, Giulia Cinquegrana, Amanda Karakas, Jamie Tayar, Dóra Tarczay-Nehéz
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2024-01-01
Collection:The Astrophysical Journal
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Accès en ligne:https://doi.org/10.3847/1538-4357/ad534a
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