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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4389
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dc.contributor.authorSharma, D. P-
dc.contributor.authorNagaraja, B. V-
dc.contributor.authorBhattacharyya, J. C-
dc.contributor.authorMohin, S-
dc.contributor.authorRaveendran, A. V-
dc.date.accessioned2009-03-05T16:47:56Z-
dc.date.available2009-03-05T16:47:56Z-
dc.date.issued1983-09-
dc.identifier.citationAstrophysics and Space Science, Vol. 95, No. 1, pp. 65 - 77en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4389-
dc.description.abstractWe have monitored the X-ray source X-Per (4U 0352+30) on 31 August, 1979 through aU filter for about 1.5 hr using 102-cm telescope of Kavalur observatory. During this period intensity of X-Per fluctuated for some time, on time scales of few minutes but recovered in the end. It was again monitored from 27 December, 1979 to January 1980 through a standardU, B, V photometer attached to a 34-cm telescope. In this paper we present the data on the fast flickerings observed on 31 August, 1979 and on the long term monitoring from December 1979 to January 1980.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00661156en
dc.subjectB Starsen
dc.subjectBinary Starsen
dc.subjectLight Curveen
dc.subjectVariable Starsen
dc.subjectX Ray Sourcesen
dc.subjectPulsarsen
dc.subjectStellar Magnitudeen
dc.subjectStellar Oscillationsen
dc.subjectUBV Spectraen
dc.titleObservations of X-Per in optical domainen
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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