Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(476), p. 3729-3743, 2018
DOI: 10.1093/mnras/sty268
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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
Journal article published in 2018 by
K. Brogaard 
,
C. J. Hansen,
A. Miglio ,
D. Slumstrup ,
S. Frandsen,
J. Jessen-Hansen,
M. N. Lund ,
D. Bossini,
A. Thygesen,
G. R. Davies,
W. J. Chaplin ,
T. Arentoft,
H. Bruntt,
F. Grundahl,
R. Handberg
,
C. J. Hansen,
A. Miglio ,
D. Slumstrup ,
S. Frandsen,
J. Jessen-Hansen,
M. N. Lund ,
D. Bossini,
A. Thygesen,
G. R. Davies,
W. J. Chaplin ,
T. Arentoft,
H. Bruntt,
F. Grundahl,
R. Handberg
This paper was not found in any repository, but could be made available legally by the author.
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