First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her

We report the first asteroseismic results obtained with the Hertzsprung SONG Telescope from an extensive high-precision radial-velocity observing campaign of the subgiant muHerculis. The data set was collected during 215 nights in 2014 and 2015. We detected a total of 49 oscillation modes with l val...

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Veröffentlicht in:arXiv.org 2017-01
Hauptverfasser: Grundahl, F, Andersen, M Fredslund, Christensen-Dalsgaard, J, Antoci, V, Kjeldsen, H, Handberg, R, Houdek, G, Bedding, T R, Pallé, P L, Jessen-Hansen, J, V Silva Aguirre, White, T R, Frandsen, S, Albrecht, S, Andersen, M I, Arentoft, T, Brogaard, K, Chaplin, W J, Harpsøe, K, Jørgensen, U G, Karovicova, I, Karoff, C, P Kjærgaard Rasmussen, Lund, M N, Lundkvist, M Sloth, Skottfelt, J, A Norup Sørensen, Tronsgaard, R, Weiss, E
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Sprache:eng
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Zusammenfassung:We report the first asteroseismic results obtained with the Hertzsprung SONG Telescope from an extensive high-precision radial-velocity observing campaign of the subgiant muHerculis. The data set was collected during 215 nights in 2014 and 2015. We detected a total of 49 oscillation modes with l values from 0 to 3, including some l = 1 mixed modes. Based on the rotational splitting observed in l = 1 modes, we determine a rotational period of 52 days and a stellar inclination angle of 63 degrees. The parameters obtained through modeling of the observed oscillation frequencies agree very well with independent observations and imply a stellar mass between 1.11 and 1.15M_sun and an age of 7.8+/-0.4 Gyr. Furthermore, the high-quality data allowed us to determine the acoustic depths of the He II ionization layer and the base of the convection zone.
ISSN:2331-8422
DOI:10.48550/arxiv.1701.03365