Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4286
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dc.contributor.authorPeraiah, A-
dc.contributor.authorSrinivasa Rao, M-
dc.date.accessioned2009-01-24T11:57:45Z-
dc.date.available2009-01-24T11:57:45Z-
dc.date.issued1983-09-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 4, No. 3, pp. 183 - 189en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4286-
dc.description.abstractThe effects of reflection on the formation of spectral lines is investigated. The authors have assumed a purely scattering atmosphere and studied how the equivalent widths change due to irradiation from the secondary. Generally, the flux in the lines is increased at all frequency points, the cores of the lines receiving more flux than the wings. Moreover, the proximity of the secondary component changes the equivalent widths considerably. The further away the secondary is from the primary the higher are the equivalent widths.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://dx.doi.org/10.1007/BF02714905en
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4..183Pen
dc.subjectReflection Effect - Spectral Line Formationen
dc.titleReflection effect in close binaries. V. effects of reflection on spectral line formationen
dc.typeArticleen
Appears in Collections:IIAP Publications

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