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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3017
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dc.contributor.authorKutty, K. R. N-
dc.contributor.authorMarar, T. M. K-
dc.contributor.authorPadmini, V. N-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.contributor.authorRao, U. R-
dc.contributor.authorBhattacharyya, J. C-
dc.contributor.authorMohin, S-
dc.contributor.authorJayakumar, K-
dc.date.accessioned2008-08-05T07:39:20Z-
dc.date.available2008-08-05T07:39:20Z-
dc.date.issued1986-
dc.identifier.citationHydrogen deficient stars and related objects; Proceedings of the Eighty-seventh IAU Colloquium, pp. 397 - 402en
dc.identifier.urihttp://hdl.handle.net/2248/3017-
dc.description.abstractWe report fast photometric observations of AM Canum Venaticorum (AM CVn), the ultrashort-period, hydrogen-deficient variable, are reported. An intense flare of (Delta m) peak roughly 0.34 was detected on February 24th, 1985 in white light lasting over 200 s. Following this flare, an enhanced double-humped structure lasting for 1051 s was observed which is the dominant periodicity exhibited by AM CVn. The 525 s and 1051 s periods were also detected. In addition, the authors report flickerings lasting typically 1-2 minutes that are characteristic of cataclysmic variables.en
dc.format.extent133321 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.subjectCataclysmic variablesen
dc.subjectStellar activityen
dc.subjectStellar spectrophotometryen
dc.subjectWhite dwarf starsen
dc.subjectLight curveen
dc.subjectSpectral energy distributionen
dc.subjectStellar flaresen
dc.titleDetection of an extremely active state of AM Canum Venaticorumen
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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