Asteroseismological calibration of open clusters

dc.contributor.author	Audard, N
dc.contributor.author	Brown, T. M
dc.contributor.author	Christensen-Dalsgaard, J
dc.contributor.author	Frandsen, S
dc.contributor.author	Kjeldsen, H
dc.date.accessioned	2007-09-19T11:41:21Z
dc.date.available	2007-09-19T11:41:21Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 305-308	en
dc.identifier.uri	http://hdl.handle.net/2248/1813
dc.description.abstract	Combining classical and seismological data permits one to perform a calibration of stars, and therefore to improve the estimate of their fundamental parameters. We present preliminary results of the calibration of stars in the Hyades open cluster, using the SVD formalism. This permits us to see which are the most important observables for estimating stellar parameters. The analysis will help to optimize possible experiments and to improve the stellar modelling. It will also be useful for the choice of targets for the future seismic space mission STARS.	en
dc.format.extent	343796 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..305A	en
dc.subject	Stars: oscillations	en
dc.subject	Open clusters: Hyades	en
dc.title	Asteroseismological calibration of open clusters	en
dc.type	Article	en