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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1576
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dc.contributor.authorPadalia, T. D-
dc.contributor.authorGupta, S. K-
dc.contributor.authorSrivastava, R. K-
dc.contributor.authorChaubey, U. S-
dc.date.accessioned2007-05-10T06:13:09Z-
dc.date.available2007-05-10T06:13:09Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 647-649en
dc.identifier.urihttp://hdl.handle.net/2248/1576-
dc.description.abstractThe comet Swift-Tuttle (1992t) was observed through UBV filters during twelve nights in December 1992. Magnitude variations of six circular zones from the center of the cometary head have been given. On the night of 17 December 1992, sharp magnitude variations have been noticed in all the three filters during a span of one hour of observationsen
dc.format.extent193265 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectCometen
dc.subjectUBV photometryen
dc.titleUBV photometry of comet Swift-Tuttle (1992t)en
dc.typeArticleen
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