Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4287
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dc.contributor.authorPeraiah, A-
dc.contributor.authorSrinivasa Rao, M-
dc.date.accessioned2009-01-24T12:03:31Z-
dc.date.available2009-01-24T12:03:31Z-
dc.date.issued1983-09-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 4, No. 3, pp. 175 - 189en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4287-
dc.description.abstractThe law of limb darkening has been calculated when the atmosphere of the primary component is illuminated by the extended surface of the secondary component in a binary system. The specific intensities calculated at infinity show marked changes when the plane-parallel approximation is replaced by the assumption of spherical symmetry. The middle portions of the illuminated surface reflect maximum radiation while the innermost and outermost layers show lesser amount of reflected radiation.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4..175Pen
dc.relation.urihttp://www.springerlink.com/content/e86283751k322575/en
dc.subjectReflection Effect - Limb Darkeningen
dc.titleReflection effect in close binaries. IV - Limb darkening of the reflected radiation incident from an extended surface of the secondaryen
dc.typeArticleen
Appears in Collections:IIAP Publications

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