A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology

Context. Asteroseismic modelling of the internal structure of main-sequence stars born with a convective core has so far been based on homogeneous analyses of space photometric Kepler light curves of four years in duration, to which most often incomplete inhomogeneously-deduced spectroscopic informa...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-06, Vol.650, p.A151
Hauptverfasser:	Gebruers, Sarah, Straumit, Ilya, Tkachenko, Andrew, Mombarg, Joey S. G., Pedersen, May G., Van Reeth, Timothy, Li, Gang, Lampens, Patricia, Escorza, Ana, Bowman, Dominic M., De Cat, Peter, Vermeylen, Lore, Bodensteiner, Julia, Rix, Hans-Walter, Aerts, Conny
Format:	Artikel
Sprache:	eng
Schlagworte:	Abundance Astronomical models Atmospheric models B stars F stars Light curve Machine learning Main sequence stars Metallicity Microprocessors Parameters Space telescopes Spectrum analysis Stellar evolution Stellar models Stellar rotation Stellar seismology
Online-Zugang:	Volltext
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