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Reflection effect in close binaries. III - Distribution of radiation incident from an extended source

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dc.contributor.author Peraiah, A
dc.date.accessioned 2009-01-16T14:10:40Z
dc.date.available 2009-01-16T14:10:40Z
dc.date.issued 1983-06
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 4, pp. 151 - 159 en
dc.identifier.issn 0250-6335
dc.identifier.uri http://hdl.handle.net/2248/4262
dc.description.abstract The 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.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://adsabs.harvard.edu/abs/1983JApA....4..151P en
dc.rights © Indian Academy of Sciences en
dc.subject Binary Stars en
dc.subject Electron Density Profiles en
dc.subject Radiative Transfer en
dc.subject Stellar Atmospheres en
dc.subject Wave Reflection en
dc.subject Angular Distribution en
dc.subject Electron Scattering en
dc.subject Incident Radiation en
dc.subject Point Sources en
dc.title Reflection effect in close binaries. III - Distribution of radiation incident from an extended source en
dc.type Article en


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