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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3653
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dc.contributor.authorPeraiah, A-
dc.contributor.authorIngalgi, M. F-
dc.date.accessioned2008-09-16T14:26:44Z-
dc.date.available2008-09-16T14:26:44Z-
dc.date.issued1990-06-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 11, No.2, pp. 209 - 219en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3653-
dc.description.abstractThe profiles of hydrogen Lyman-alpha line in an expanding spherical atmosphere containing dust and gas were calculated. The variation of equivalent widths with velocities of expansion of the atmosphere, together with the amount of dust present in the medium is being investigated. Curves of growth have been drawn for different velocities and dust optical depths.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1990JApA...11..209Pen
dc.subjectComputational astrophysicsen
dc.subjectH linesen
dc.subjectLyman alpha radiationen
dc.subjectSpectral line widthen
dc.subjectStellar atmospheresen
dc.subjectAbsorption spectraen
dc.subjectCosmic dusten
dc.subjectLine spectraen
dc.subjectStellar envelopesen
dc.subjectStellar spectraen
dc.titleEquivalent widths of hydrogen Lyman alpha line in an expanding spherical atmosphereen
dc.typeArticleen
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