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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/585
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dc.contributor.authorShah, Ghanshyam, A-
dc.date.accessioned2005-12-05T07:04:23Z-
dc.date.available2005-12-05T07:04:23Z-
dc.date.issued1983-03-
dc.identifier.citationBASI, Vol. 11, No. 1, pp. 63-69en
dc.identifier.urihttp://hdl.handle.net/2248/585-
dc.descriptionOpen Access-
dc.description.abstractThe phase retardation by cylindrical grains composed of pure (index of refraction, m=1.33 - i0.0) and dirty (m = 1.33 - i0.05) ice materials has been investigated. It has been found that the resulting interstellar circular polarization is likely to be more pronounced in the near-and far-infrared wavelength regions. The orientation of the grains, even in the case of dielectric materials, plays an important role in producing interstellar circular polarization.en
dc.format.extent531308 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectInterstellar grainsen
dc.subjectInterstellar circular polarizationen
dc.subjectPhase retaradtionen
dc.subjectScattering of lighten
dc.titlePhase retardation of light due to scattering by interstellar nonspherical grainsen
dc.typeArticleen
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