Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3673
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dc.contributor.authorSen, A. K-
dc.contributor.authorJoshi, U. C-
dc.contributor.authorDeshpande, M. R-
dc.contributor.authorBabu, G. S. D-
dc.contributor.authorKulshrestha, A. K-
dc.date.accessioned2008-09-16T16:02:27Z-
dc.date.available2008-09-16T16:02:27Z-
dc.date.issued1988-10-
dc.identifier.citationAstronomy and Astrophysics , Vol. 204, No. 1 - 2, pp. 317 - 318en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3673-
dc.description.abstractOptical linear polarization data are presented for the coma and tail region of comet P/Halley observed on 19 March 1986. Polarization in the continuum has been found to increase with wavelength while the position angle remains almost constant. The nature of the wavelength dependence of polarization seems to be different for the coma and the tail region, signifying a size difference of the particles in the two regions. The wavelength dependence of polarization shows a decrease in polarization across different emission bands (CN, C3, CO+, C2 and H2O+).en
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1988A%26A...204..317Sen
dc.subjectComet Tailsen
dc.subjectHalley's Cometen
dc.subjectLinear Polarizationen
dc.subjectMolecular Ionsen
dc.subjectSpectral Bandsen
dc.subjectCarbon Monoxideen
dc.subjectCN Emissionen
dc.subjectEmission Spectraen
dc.subjectWater Vaporen
dc.titlePolarimetric observations of comet P/Halley on 19 March 1986en
dc.typeArticleen
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