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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4202
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dc.contributor.authorSharma, D. P-
dc.contributor.authorMarar, T. M. K-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.contributor.authorRao, U. R-
dc.contributor.authorBhattacharyya, J. C-
dc.date.accessioned2008-12-29T14:35:39Z-
dc.date.available2008-12-29T14:35:39Z-
dc.date.issued1983-08-
dc.identifier.citationInternational Cosmic Ray Conference, 18th, Bangalore, India, Aug 22 - Sept 3, 1983, Vol. 9, pp. 330 - 333en
dc.identifier.urihttp://hdl.handle.net/2248/4202-
dc.description.abstractHigh speed optical photometric observations of the hard X-ray source EX Hya, carried out with the reflector of the Kevalur Observatory, are presented. The observations with time resolutions of 1 s or 2 s were made on four nights in March 1982 for a total duration of 6.8 h. Light curves that reveal fast flickerings and the 67 min oscillations are presented. A new ephemeris for the photometric period confirms the trend towards decreasing period on a time scale of 10-million years. Evidence for the presence of interpulses in the light curves between successive photometric maximaen
dc.language.isoenen
dc.publisherINSDOCen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983ICRC....9..330Sen
dc.subjectDwarf Novaeen
dc.subjectLight Curveen
dc.subjectStellar Spectrophotometryen
dc.subjectX Ray Sourcesen
dc.subjectEclipsing Binary Starsen
dc.subjectHigh Resolutionen
dc.subjectWhite Dwarf Starsen
dc.titleHigh speed photometry of dwarf nova EX Hydraeen
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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