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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/170
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dc.contributor.authorKrishna Swamy, K. S-
dc.contributor.authorShah, G. A-
dc.date.accessioned2004-12-28T07:09:55Z-
dc.date.available2004-12-28T07:09:55Z-
dc.date.issued1988-08-
dc.identifier.citationMonthly Notices Royal Astronomical Society, Vol. 233, pp. 573 – 579en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/170-
dc.description.abstractThe observed reddening in the wavelength range 0.26-2.25 microns for comae of several comets can be represented quite well with model grains having real and imaginary parts of refractive index, m = m-prime - im-double prime, given by m-prime of about 1.38 and m-double prime of about 0.039, respectively. It is also possible to explain the observations of linear polarization and geometric albedo of comet comae-
dc.format.extent244020 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1988MNRAS.233..573K-
dc.subjectAlbedoen
dc.subjectCometary Atmospheresen
dc.subjectCosmic Dusten
dc.subjectLight Scatteringen
dc.subjectLinear Polarizationen
dc.titleNature of dust grains in cometsen
dc.typeArticleen
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