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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2054
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-02-26T07:26:58Z-
dc.date.available2008-02-26T07:26:58Z-
dc.date.issued1990-02-
dc.identifier.citationAstrophysics and Space Science, Vol. 164, No. 1, pp. 63 - 67en
dc.identifier.urihttp://hdl.handle.net/2248/2054-
dc.description.abstractThe spectrophotometric and photometric observations of the WC star HD 76536 are reported. The flux and the magnitude variations appear to be periodic. The possibilities of a compact binary are discussed.en
dc.format.extent132205 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishers-
dc.relation.urihttp://dx.doi.org/10.1007/BF00653550en
dc.relation.urihttp://adsabs.harvard.edu/abs/1990Ap%26SS.164...63S-
dc.subjectAtomic Physicsen
dc.subjectBinary Stars-
dc.subjectStellar Spectrophotometry-
dc.subjectVariable Stars-
dc.subjectEmission Spectra-
dc.subjectLight Curve-
dc.subjectStellar Magnitude-
dc.titleThe variability of HD 76536en
dc.typeArticleen
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