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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2262
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dc.contributor.authorSaha, S. K-
dc.contributor.authorJayarajan, A. P-
dc.contributor.authorSudheendra, G-
dc.contributor.authorChandra, A. U-
dc.date.accessioned2008-04-24T11:24:17Z-
dc.date.available2008-04-24T11:24:17Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 3, pp. 379 - 387en
dc.identifier.urihttp://hdl.handle.net/2248/2262-
dc.description.abstractAn interferometer system for use at the 2.34 meter Vainu Bappu Telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur, to obtain speckle-grams of astronomical objects in the visible wavelength, has been developed. Laboratory tests of resultant intensity distributions due to a point source, with phase modulation screens, as well as the images obtained using this interferometer at the cassegrain end of the said telescope are discusseden
dc.format.extent831261 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..379Sen
dc.subjectInterferometeren
dc.subjectSpeckleen
dc.subjectBinaryen
dc.titlePerformance of a speckle interferometeren
dc.typeArticleen
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