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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/962
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dc.contributor.authorShah, G. A-
dc.date.accessioned2006-04-13T04:56:56Z-
dc.date.available2006-04-13T04:56:56Z-
dc.date.issued1989-09-
dc.identifier.citationBASI, Vol. 17, No. 3, pp. 114-119en
dc.identifier.urihttp://hdl.handle.net/2248/962-
dc.description.abstractA new relation between the nuclear radius and the optical depth toward the nucleus of Comet Halley has been derived on the basis of the radial variation of the effective area of the grains along the Giotto trajectory in the coma. It is found that the expected optical depth toward the nucleus varies from 0.089 to 0.036 corresponding to the nuclear radius in the range 8 to 16 km.en
dc.format.extent401424 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectComet Halleyen
dc.subjectDust grainsen
dc.subjectNucleusen
dc.subjectOptical depth in comaen
dc.titleOptical depth towards the nucleus of Halley's cometen
dc.typeArticleen
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