Projects per year
Abstract
Convective mixing in Helium-core-burning (HeCB) stars is one of the outstanding issues in stellar modelling. The precise asteroseismic measurements of gravity-modes period spacing (ΔΠ1) has opened the door to detailed studies of the near-core structure of such stars, which had not been possible before. Here we provide stringent tests of various core-mixing scenarios against the largely unbiased population of red-clump stars belonging to the old open clusters monitored by Kepler, and by coupling the updated precise inference on ΔΠ1 in thousands field stars with spectroscopic constraints. We find that models with moderate overshooting successfully reproduce the range observed of ΔΠ1 in clusters. In particular we show that there is no evidence for the need to extend the size of the adiabatically stratified core, at least at the beginning of the HeCB phase. This conclusion is based primarily on ensemble studies of ΔΠ1 as a function of mass and metallicity. While ΔΠ1 shows no appreciable dependence on the mass, we have found a clear dependence of ΔΠ1 on metallicity, which is also supported by predictions from models.
Original language | English |
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Journal | Royal Astronomical Society. Monthly Notices |
Early online date | 10 May 2017 |
DOIs | |
Publication status | E-pub ahead of print - 10 May 2017 |
Keywords
- Astrophysics - Astrophysics of Galaxies
- stars: evolution
- asteroseismology
- stars: low-mass
- stars: interiors
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Dive into the research topics of 'Kepler red-clump stars in the field and in open clusters: constraints on core mixing'. Together they form a unique fingerprint.Projects
- 1 Finished
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Asteroseismology and Helioseismology at Birmingham and Queen Mary
Chaplin, B., Elsworth, Y. & Miglio, A.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/15 → 30/09/18
Project: Research Councils