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Comparison of wavelength dependent giant star angular diameters with models

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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


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