Cool star flux spectra for population studies in galaxies

dc.contributor.author	Malagnini, M. L
dc.contributor.author	Morossi, C
dc.contributor.author	Buser, R
dc.contributor.author	Parthasarathy, M
dc.date.accessioned	2008-06-26T10:28:45Z
dc.date.available	2008-06-26T10:28:45Z
dc.date.issued	1992-08
dc.identifier.citation	A&A, Vol. 264, No. 2, pp. 558 - 564	en
dc.identifier.uri	http://hdl.handle.net/2248/2512
dc.description.abstract	Five solar-composition cool giant stars have been observed with the IUE low resolution mode. The UV energy distributions were merged with visual spectrophotometry from the literature and compared with predictions from two new grids of model atmospheres. Atmospheric parameters were derived consistent with the literature data by matching observations and models in the optical region. Significant discrepancies between data and model predictions found in the IUE ultraviolet region are illustrated and briefly discussed	en
dc.format.extent	829479 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	EDP Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1992A%26A...261..558M	en
dc.subject	COOL STARS	en
dc.subject	GALAXIES	en
dc.subject	GIANT STARS	en
dc.subject	IUE	en
dc.subject	SPECTRAL ENERGY DISTRIBUTION	en
dc.subject	STELLAR EVOLUTION	en
dc.subject	STELLAR SPECTROPHOTOMETRY	en
dc.title	Cool star flux spectra for population studies in galaxies	en
dc.type	Article	en