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Results from the PTI's studies of the spectral angular diameters of Mira variables

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dc.contributor.author Thompson, R. R. en_US
dc.contributor.author Creech-Eakman, M. J. en_US
dc.contributor.author Belle, G. T. van en_US
dc.date.accessioned 2004-09-20T19:49:59Z
dc.date.available 2004-09-20T19:49:59Z
dc.date.issued 2002-08-22 en_US
dc.identifier.citation SPIE Astronomical Telescopes and Instrumentation en_US
dc.identifier.citation Waikoloa, HI, USA en_US
dc.identifier.clearanceno 02-3181 en_US
dc.identifier.uri http://hdl.handle.net/2014/11239
dc.description.abstract A dedicated program of measuring angular sizes of Mira variables using the Palomar Testbed Interferometer has resulted in more than 13,000 measurements of over 60 stars. en_US
dc.format.extent 3292436 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other interferometry Miras stellar diameters near-infrared stellar atmospheres spectroscopy oscillations stellar chemistry en_US
dc.title Results from the PTI's studies of the spectral angular diameters of Mira variables en_US


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