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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2512
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dc.contributor.authorMalagnini, M. L-
dc.contributor.authorMorossi, C-
dc.contributor.authorBuser, R-
dc.contributor.authorParthasarathy, M-
dc.date.accessioned2008-06-26T10:28:45Z-
dc.date.available2008-06-26T10:28:45Z-
dc.date.issued1992-08-
dc.identifier.citationA&A, Vol. 264, No. 2, pp. 558 - 564en
dc.identifier.urihttp://hdl.handle.net/2248/2512-
dc.description.abstractFive 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 discusseden
dc.format.extent829479 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992A%26A...261..558Men
dc.subjectCOOL STARSen
dc.subjectGALAXIESen
dc.subjectGIANT STARSen
dc.subjectIUEen
dc.subjectSPECTRAL ENERGY DISTRIBUTIONen
dc.subjectSTELLAR EVOLUTIONen
dc.subjectSTELLAR SPECTROPHOTOMETRYen
dc.titleCool star flux spectra for population studies in galaxiesen
dc.typeArticleen
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