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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3804
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dc.contributor.authorMohan Rao, D-
dc.contributor.authorRangarajan, K. E-
dc.contributor.authorPeraiah, A-
dc.date.accessioned2008-09-23T10:00:47Z-
dc.date.available2008-09-23T10:00:47Z-
dc.date.issued1984-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 5, No. 2, pp. 169 - 180en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3804-
dc.description.abstractThe effects of partial frequency redistribution on the formation of spectral lines have been studied. The angle-averaged R(II), R(III) and R(V) types of redistribution with isotropic phase function have been considered. Transfer equation with plane-parallel geometry is solved in isothermal atmospheres. For an atmosphere with constant thermal sources, the frequency-dependent source function S/L/(R/V/) lies below S/L/(R/III/) but above S/L/(R/II/) in the line wings.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1984JApA....5..169Men
dc.subjectAtmospheric Modelsen
dc.subjectFrequency Distributionen
dc.subjectLine Spectraen
dc.subjectRadiative Transferen
dc.subjectStellar Atmospheresen
dc.titleEffects of partial frequency redistribution functions R(II), R(III) and R(V) on source functionsen
dc.typeArticleen
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