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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1431
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dc.contributor.authorMekkaden, M. V-
dc.date.accessioned2007-03-14T08:49:25Z-
dc.date.available2007-03-14T08:49:25Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 351-355en
dc.identifier.urihttp://hdl.handle.net/2248/1431-
dc.description.abstractUBVRI photometry of the isolated T Tauri star TW Hya, obtained during 1987 April from ESO, is presented. The data analysis shows a periodicity of 2.195 d in light variation. The steep increase of amplitude towards shorter wavelengths is interpreted as due to the rotational modulation of hot plage region on the stellar surfaceen
dc.format.extent145208 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectT Tauri staren
dc.subjectUBVRIen
dc.titlePeriodic activity in the T Tauri star TW Hyaen
dc.typeArticleen
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