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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4863
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dc.contributor.authorMohin, S-
dc.contributor.authorRaveendran, A. V-
dc.contributor.authorMekkaden, M. V-
dc.date.accessioned2009-10-16T10:59:57Z-
dc.date.available2009-10-16T10:59:57Z-
dc.date.issued1995-
dc.identifier.citationStrassmeier, K. G. ed., Stellar surface structure: poster proceedings, Proceedings of IAU symposium 176, Vienna, Austria, 9 - 13 october, 1995, pp. 84 - 86en
dc.identifier.isbn3-901617-01-9-
dc.identifier.urihttp://hdl.handle.net/2248/4863-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.ispartofseriesInternational Astronomical Union Symposium;Vol. 176-
dc.relation.urihttp://adsabs.harvard.edu//abs/1995IAUS..176P..84Men
dc.rights© International Astronomical Unionen
dc.subjectLong Term Photometricen
dc.subjectThe Active RS CVn Binariesen
dc.subjectPhotometric Variationsen
dc.subjectStellar Astrophysicsen
dc.subjectStellar Structureen
dc.titleLong-term photometric variations of the active RS CVn binaries DM UMa and II Pegen
dc.typeArticleen
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