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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/577
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2005-08-27T04:40:09Z-
dc.date.available2005-08-27T04:40:09Z-
dc.date.issued1985-04-
dc.identifier.citationAstrophysics and Space Science. Vol. 111, No. 2, pp. 407 – 411en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/577-
dc.description.abstractPhotometric observations of EX Hya in B and V filters are reported. The 67 min modulation of the light curve is also found to be in good agreement with the results of earlier studies. The (B-V) colour variation with respect to the 67 min variation is found to be opposite to those of typical colour variation during hump/superhump activity in other dwarf novae. The model of an intermediate polar is discussed.-
dc.format.extent7229 bytes-
dc.format.mimetypetext/html-
dc.language.isoen-
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1985Ap%26SS.111..407S-
dc.relation.urihttp://dx.doi.org/10.1007/BF00649980-
dc.subjectCataclysmic Variables-
dc.subjectDwarf Novae-
dc.subjectLight Curve-
dc.subjectStellar Color-
dc.subjectStellar Spectrophotometry-
dc.subjectStellar Models-
dc.subjectWhite Dwarf Stars-
dc.titlePhotometry of EX Hyaen
dc.typeArticleen
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