Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4173
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dc.contributor.authorSeetha, S-
dc.contributor.authorMarar, T. M. K-
dc.contributor.authorSharma, D. P-
dc.contributor.authorKasturirangan, K-
dc.contributor.authorRao, U. R-
dc.contributor.authorBhattacharyya, J. C-
dc.date.accessioned2008-12-29T11:45:14Z-
dc.date.available2008-12-29T11:45:14Z-
dc.date.issued1983-08-
dc.identifier.citationProceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 Aug - 3 Sept, 1983, Vol. 9, pp. 5 - 8en
dc.identifier.urihttp://hdl.handle.net/2248/4173-
dc.description.abstractHigh speed optical photometric observations of the X-ray dwarf nova HL Canis Majoris (1E 0643-1648), discovered with the Einstein Observatory, are presented. Results of long term monitoring and attempts to detect photometric eclipses at the reported orbital periods of 0.22 d or 0.18 d of the binary system are presented.en
dc.language.isoenen
dc.publisherINSDOCen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983ICRC....9....5Sen
dc.subjectPhotometric Observationsen
dc.subjectX-Ray Dwarf Nova HL Canis Majorisen
dc.titlePhotometric Observations of the X-Ray Dwarf Nova HL Canis Majorisen
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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