Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2585
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dc.contributor.authorAshoka, B. N-
dc.contributor.authorMarar, T. M. K-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.contributor.authorBhattacharyya, J. C-
dc.date.accessioned2008-07-09T07:29:36Z-
dc.date.available2008-07-09T07:29:36Z-
dc.date.issued1995-05-
dc.identifier.citationAstronomy and Astrophysics, Vol. 297, No. 3, pp. L83 – L86en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2585-
dc.description.abstractWe report the detection of optical pulsations at a period of 272.785+-0.003s from the newly discovered intermediate polar RX J0558.0+5353. This period nearly coincides with the X-ray period reported by Haberl et al. (1994). In the optical band the folded light curve of the star reveals a non-sinusoidal pulse with a pulsed fraction of 10.8%.en
dc.format.extent473044 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe European Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995A%26A...297L..83Aen
dc.subjectBinaries: Closeen
dc.subjectStars: Individual: Rx J0558.0+5353en
dc.subjectStars: Cataclysmic Variablesen
dc.subjectX-Rays: Starsen
dc.titleDetection of optical pulsations from RX J0558.0+5353en
dc.typeArticleen
Appears in Collections:J.C.Bhattacharyya (1982 - 1990)
IIAP Publications

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