Asteroseismic Structure Inversions of Main-sequence Solar-like Oscillators with Convective Cores

Asteroseismic Structure Inversions of Main-sequence Solar-like Oscillators with Convective Cores

Asteroseismic inferences of main-sequence solar-like oscillators often rely on best-fit models. However, these models cannot fully reproduce the observed mode frequencies, suggesting that the internal structure of the model does not fully match that of the star. Asteroseismic structure inversions pr...

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Bibliographic Details
Main Authors: Lynn Buchele, Earl P. Bellinger, Saskia Hekker, Sarbani Basu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Asteroseismology
Stellar physics
Stellar structures
Stellar evolutionary models
Stellar oscillations
Online Access:https://doi.org/10.3847/1538-4357/add697
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https://doi.org/10.3847/1538-4357/add697

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