Establishing the accuracy of asteroseismic mass and radius estimates of giant stars – I. Three eclipsing systems at [Fe/H] ∼ −0.3 and the need for a large high-precision sample-Reference-Cited by-同舟云学术

Establishing the accuracy of asteroseismic mass and radius estimates of giant stars – I. Three eclipsing systems at [Fe/H] ∼ −0.3 and the need for a large high-precision sample

Published:2018-02-01 Issue:3 Volume:476 Page:3729-3743
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Brogaard K¹²^ORCID,Hansen C J³,Miglio A¹²,Slumstrup D²^ORCID,Frandsen S²,Jessen-Hansen J²,Lund M N¹²^ORCID,Bossini D¹,Thygesen A⁴,Davies G R¹²,Chaplin W J¹²,Arentoft T²,Bruntt H²,Grundahl F²,Handberg R²^ORCID

Affiliation:

1. School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

2. Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

3. Dark Cosmology Centre, The Niels Bohr Institute, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

4. California Institute of Technology, 1200 E. California Blvd., MC 249-17, Pasadena, CA 91125, USA

Funder

National Research Foundation

European Research Council

NASA

Publisher

Oxford University Press (OUP)

Subject