Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4262
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dc.contributor.authorPeraiah, A-
dc.date.accessioned2009-01-16T14:10:40Z-
dc.date.available2009-01-16T14:10:40Z-
dc.date.issued1983-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 4, pp. 151 - 159en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4262-
dc.description.abstractThe effects of irradiation from an extended surface of the secondary component on the atmosphere of the primary are studied. Consideration is given to an isothermal and purely scattering medium. The resultant radiation field due to irradiation from an extended surface and self-radiation is different from that due to irradiation from a point source and self-radiation. In the case of the point source the middle layers of the exposed part of the atmosphere show maximum reflection, while in the former case the reflection gradually decreases from the center of the component towards the surface of the outermost layers of the atmosphere. The reflection effect appears to be strongly dependent on the density distribution of the electrons.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4..151Pen
dc.rights© Indian Academy of Sciencesen
dc.subjectBinary Starsen
dc.subjectElectron Density Profilesen
dc.subjectRadiative Transferen
dc.subjectStellar Atmospheresen
dc.subjectWave Reflectionen
dc.subjectAngular Distributionen
dc.subjectElectron Scatteringen
dc.subjectIncident Radiationen
dc.subjectPoint Sourcesen
dc.titleReflection effect in close binaries. III - Distribution of radiation incident from an extended sourceen
dc.typeArticleen
Appears in Collections:IIAP Publications

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