Asteroseismic analysis of solar-mass subgiants KIC 6442183 and KIC 11137075 observed byKepler

2015/06/05 by Zhijia Tian, Shaolan Bi, Timothy R. Bedding +1 · 1 citation
Physics and Astronomy · Social Sciences · #Asteroseismology #Astronomy and Astrophysical Research #Educational Leadership and Practices #Stars #Starspot #Statistical analysis #Stellar evolution #Stellar, planetary, and galactic studies #Subgiant #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201525968

published as A&A 580, A44 (2015) · 9 pages, 8 figures, 5 tables A&A accepted

arxiv created 2015/06/05 · openalex publication_date 2015/06/24 · arxiv updated 2015/07/29 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

Context. Asteroseismology provides a powerful way to constrain stellar parameters. Solar-like oscillations have been observed on subgiant stars with the Kepler mission. The continuous and high-precision time series enables us to carry out a detailed asteroseismic study for these stars.

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• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters

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