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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1577
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dc.contributor.authorJoshi, U. C-
dc.contributor.authorChauhan, J. S-
dc.contributor.authorDeshpande, M. R-
dc.contributor.authorSen, A. K-
dc.contributor.authorBhatnagar, A. K-
dc.date.accessioned2007-05-10T08:51:52Z-
dc.date.available2007-05-10T08:51:52Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 651-653en
dc.identifier.urihttp://hdl.handle.net/2248/1577-
dc.description.abstractComet Austin (1989c) was observed during April and May 1990 when its phase was between 106 deg and 110 deg. No unusual activity in the form of jet is seen in the polarization map. Polarization is low near the nucleus and high (approximately 16%) in the outer region (mean distance of 190,000 km on west side), suggesting segregation of grainsen
dc.format.extent423877 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectCometen
dc.subjectPolarimetryen
dc.titleImaging polarimetry of comet Austinen
dc.typeArticleen
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