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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/672
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2006-01-05T04:10:46Z-
dc.date.available2006-01-05T04:10:46Z-
dc.date.issued1984-10-
dc.identifier.citationAstrophysics and Space Science, Vol. 104, No. 1, pp. 163 - 168en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/672-
dc.description.abstractSpectrophotometric observations of Nova Coronae Austrinae 1981, during its nebular phase are reported. The various emission lines are identified. The electron densities and the mass of the ionized hydrogen in the shell have been calculated. The excess flux in the red continuum probably indicates the appearance of the dust component.en
dc.format.extent898771 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS.104..163S-
dc.relation.urihttp://dx.doi.org/10.1007/BF00654002-
dc.subjectNovaeen
dc.subjectSpectrum Analysis-
dc.subjectStellar Spectrophotometry-
dc.subjectBlack Body Radiation-
dc.subjectElectron Density (Concentration)-
dc.subjectEmission Spectra-
dc.subjectHydrogen Ions-
dc.subjectLine Spectra-
dc.subjectStellar Envelopes-
dc.subjectIon Density (Concentration)-
dc.titleSpectrophotometry of Nova Coronae Austrinae, 1981en
dc.typeArticleen
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