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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3879
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dc.contributor.authorMohin, S-
dc.contributor.authorRaveendran, A. V-
dc.contributor.authorMekkaden, M. V-
dc.date.accessioned2008-09-24T14:40:03Z-
dc.date.available2008-09-24T14:40:03Z-
dc.date.issued1986-
dc.identifier.citationInternational Astronomical Union Symposium, No. 118, pp. 309 - 311en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/3879-
dc.description.abstractB and V photometry of II Peg obtained at Kavalur on 39 nights during 1980 - 81, 1981 - 82 and 1984 - 85 is presented. From an analysis of the available data on this object the authors find that no two light curves agree in any of the following: shape, amplitude, phases of the light maxima and minima, mean light level, or brightness at the light maxima and minima.en
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1986IAUS..118..309Men
dc.subjectPhotometryen
dc.titlePhotometry of the Rs-Canum Binary II-PEGen
dc.typeArticleen
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