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On the stellar core physics of the 16 Cyg binary system: constraining the central hydrogen abundance using asteroseismology
Benard Nsamba, Margarida S Cunha, Catarina I S A Rocha, et al. Monthly Notices of the Royal Astronomical Society 514(1) 893 (2022) https://doi.org/10.1093/mnras/stac1370
Multi-cavity gravito-acoustic oscillation modes in stars
Convective boundary mixing in low- and intermediate-mass stars – I. Core properties from pressure-mode asteroseismology
George C Angelou, Earl P Bellinger, Saskia Hekker, et al. Monthly Notices of the Royal Astronomical Society 493(4) 4987 (2020) https://doi.org/10.1093/mnras/staa390
New parsec data base of α-enhanced stellar evolutionary tracks and isochrones – I. Calibration with 47 Tuc (NGC 104) and the improvement on RGB bump
Xiaoting Fu, Alessandro Bressan, Paola Marigo, et al. Monthly Notices of the Royal Astronomical Society 476(1) 496 (2018) https://doi.org/10.1093/mnras/sty235
Constraining convective regions with asteroseismic linear structural inversions
Rotation periods and seismic ages of KOIs – comparison with stars without detected planets fromKeplerobservations
T. Ceillier, J. van Saders, R. A. García, et al. Monthly Notices of the Royal Astronomical Society 456(1) 119 (2016) https://doi.org/10.1093/mnras/stv2622
In-depth study of 16CygB using inversion techniques
The observational signatures of convectively excited gravity modes in main-sequence stars
J. H. Shiode, E. Quataert, M. Cantiello and L. Bildsten Monthly Notices of the Royal Astronomical Society 430(3) 1736 (2013) https://doi.org/10.1093/mnras/sts719
Solar-like oscillations in distant stars as seen by CoRoT : the special case of HD 42618, a solar sister