Comparison of wavelength dependent giant star angular diameters with models

van Belle, Gerard; Ciardi, David R.; Hauschildt, Peter; Scholz, Michael

dc.contributor.author	van Belle, Gerard
dc.contributor.author	Ciardi, David R.
dc.contributor.author	Hauschildt, Peter
dc.contributor.author	Scholz, Michael
dc.date.accessioned	2006-02-13T23:27:40Z
dc.date.available	2006-02-13T23:27:40Z
dc.date.issued	2004-07
dc.identifier.citation	Cool Stars 13, Hamburg, Germany, July 5-9, 2004	en
dc.identifier.clearanceno	04-1353
dc.identifier.uri	http://hdl.handle.net/2014/38589
dc.description.abstract	We present angular size measurements obtained with the Palomar testbed Interferometer. Our sample includes 82 giant stars, with spectral types between B7 and M7. These objects represent the well studied subset of giant stars observed at PTI.	en
dc.description.sponsorship	NASA	en
dc.format.extent	1391112 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US	en
dc.publisher	Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2004.	en
dc.subject	evolved stars	en
dc.subject	interferometry	en
dc.subject	stars	en
dc.subject	fundamental parameters	en
dc.title	Comparison of wavelength dependent giant star angular diameters with models	en
dc.type	Preprint	en