Interior rotation of a sample of<i>γ</i>Doradus stars from ensemble modelling of their gravity-mode period spacings
T. Van ReethInstituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D3001LeuvenBelgiumA. TkachenkoInstituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D3001LeuvenBelgiumC. AertsDepartment of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
2016en
ABI
Abstract
Context. Gamma Doradus stars (hereafter γ Dor stars) are known to exhibit gravity- and/or gravito-intertial modes that probe the inner stellar region near the convective core boundary. The non-equidistant spacing of the pulsation periods is an observational signature of the stellar evolutions and current internal structure and is heavily influenced by rotation.
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