000002755 001__ 2755
000002755 005__ 20160701171710.0
000002755 0247_ $$2DOI$$a10.1051/eas/1364061
000002755 037__ $$aASTROimport-912
000002755 100__ $$aFrandsen, S.
000002755 245__ $$aDetached Eclipsing Binaries and heartbeat stars in the Kepler field
000002755 260__ $$c2013
000002755 520__ $$aWe want to compare masses and radii of Red Giant (RG) stars derived from detached Eclipsing Binaries (dEBs) (KIC 8410637: Frandsen et al. 2013) with those derived from asteroseismology, and to classify the RG as a hydrogen- or helium-burning or as an asymptotic giant branch (AGB) star. The Kepler satellite has provided unique data, that allows asteroseismology to be carried out on RG stars. Among the many RGs are a small set of dEBs, where accurate masses and radii can be measured from an analysis of observations of the binary system.
000002755 700__ $$a Brogaard, K.
000002755 700__ $$a Beck, P. G.
000002755 700__ $$a Lampens, P.
000002755 700__ $$a Garcia, R. A.
000002755 700__ $$a Hekker, S.
000002755 700__ $$a Southworth, J.
000002755 700__ $$a Degroote, P.
000002755 773__ $$c393-394$$pEAS Publications Series$$v64$$y2013
000002755 85642 $$ahttp://esoads.eso.org/abs/2013EAS....64..393F
000002755 905__ $$apublished in
000002755 980__ $$aNONREF