Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4260
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dc.contributor.authorPeraiah, A-
dc.date.accessioned2009-01-16T14:08:09Z-
dc.date.available2009-01-16T14:08:09Z-
dc.date.issued1982-12-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 3, pp. 485 - 497en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4260-
dc.descriptionOpen Access-
dc.description.abstractThe radiation field along an irradiated surface of a component in a binary system is calculated. The source of irradiation is assumed to be a point source. This is done primarily to understand easily how the incident radiation will get changed after it is being scattered by the atmosphere. It is noticed that the maximum radiation comes from intermediate points of the atmosphere, the reason being that here there exists the combined radiation due to the star and incident radiation from the point source outside the star although both are diluted.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1982JApA....3..485Pen
dc.rights© Indian Academy of Sciencesen
dc.subjectEclipsing Binary Starsen
dc.subjectRadiative Transferen
dc.subjectReflected Wavesen
dc.subjectStellar Atmospheresen
dc.subjectStellar Radiationen
dc.subjectAtmospheric Scatteringen
dc.subjectPoint Sourcesen
dc.subjectRadiation Distributionen
dc.titleReflection effect in close binaries. I - Distribution of radiation from a point sourceen
dc.typeArticleen
Appears in Collections:IIAP Publications

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