Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/874
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dc.contributor.authorSrinivasa Rao, M-
dc.date.accessioned2006-04-08T05:35:25Z-
dc.date.available2006-04-08T05:35:25Z-
dc.date.issued2009-
dc.identifier.citationPublications of the Astronomical Observatory of Belgrade, Vol. 86, pp. 59-66en
dc.identifier.urihttp://hdl.handle.net/2248/874-
dc.description.abstractA concise description of the method of obtaining the solution of radiative trans- fer equation which can be applied to di®erent geometrical and physical systems is given. This paper mainly deals with the steps for obtaining solution of transfer equation like (1) interaction principle for di®erent geometries, (2) star product and (3) calculation of radiation field at internal points, and their applications in stellar atmosphere problems; in particular (a) study of re°ection e®ect in close binary systems and (b) stellar winds in O and B type stars are discussed with their results.-
dc.format.extent48547878 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Observatory, Volgina 7, 11160 Beograd, Serbia.en
dc.relation.urihttp://publications.aob.rs/86/pdf/059-066.pdf-
dc.rights© Astronomical Observatory, Volgina 7, 11160 Beograd, Serbia.-
dc.titleDiscrete Space Theory of Radiative Transfer: Applicationsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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