Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3843
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-09-23T14:34:13Z-
dc.date.available2008-09-23T14:34:13Z-
dc.date.issued1987-02-
dc.identifier.citationAstrophysics and Space Science , Vol. 130, No. 1 - 2, pp. 181 - 185en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/3843-
dc.description.abstractPhotometric observations of BD -7°3007 in B and V filters are reported. Rapid flickering appears to be present at all phases, implying an unfavourable angle of inclination of orbit for seeing eclipse effects. A modulation of the light curve of period about an hour is present only on one night. The continuum energy distribution agrees with that of β Com (G0 V) in the longer wavelength region only.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00654992en
dc.subjectEclipsing binary starsen
dc.subjectLight curveen
dc.subjectNovaen
dc.subjectStellar orbitsen
dc.subjectStellar spectrophotometryen
dc.subjectContinuous spectraen
dc.subjectSpectral energy distributionen
dc.titlePhotometry of BD -7 deg 3007en
dc.typeArticleen
Appears in Collections:IIAP Publications

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