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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4263
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dc.contributor.authorPeraiah, A-
dc.date.accessioned2009-01-16T14:12:58Z-
dc.date.available2009-01-16T14:12:58Z-
dc.date.issued1983-09-
dc.identifier.citationAstrophysics and Space Science , Vol. 95, No. 1, pp. 117 - 121en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4263-
dc.description.abstractThe author has calculated source functions in a scattering medium in which the density changes according to the law of Ne(r) ≡ rn where n takes the value from -3 to +3 and Ne(r) is the electron density. He has assumed that the media consist of electrons and he has also considered a geometrically extended media in which the outer radii are 2,3,5 times the inner radius. The source functions obtained are completely due to electron scattering. It is found that the source function varies considerably for different variations of density changes from n = -3 to +3.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1983Ap%26SS..95..117Pen
dc.relation.urihttp://www.springerlink.com/content/n2011nk124p13746/en
dc.rights© D. Reidel Publishing Co.en
dc.subjectElectron Density (Concentration)en
dc.subjectElectron Scatteringen
dc.subjectRadiative Transferen
dc.subjectScattering Functionsen
dc.subjectStellar Atmospheresen
dc.subjectLine Spectraen
dc.subjectOptical Thicknessen
dc.subjectStellar Spectraen
dc.titleDensity dependence of the line source functions in scattering mediaen
dc.typeArticleen
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