Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4629
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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.authorRao, U. R-
dc.contributor.authorBhattacharyya, J. C-
dc.date.accessioned2009-07-11T12:41:09Z-
dc.date.available2009-07-11T12:41:09Z-
dc.date.issued1993-
dc.identifier.citationBarstow, M. A., ed., White dwarfs: advances in observation and theory., Proceedings of the NATO Advanced Research Workshop '8th European Workshop, held in Leicester, U.K., July 20-24, 1992, NATO Advanced Science Institutes (ASI) Series C, Volume 403, pp. 537 – 541en
dc.identifier.isbn0-7923-2332-7-
dc.identifier.urihttp://hdl.handle.net/2248/4629-
dc.descriptionRestricted Access-
dc.description.abstractWe report time series photometric observations of PG 1012-029, conducted during 1990 and 1991. Light curves of three consecutive eclipses recorded in a single night are presented. The enhanced pre-eclipse hump in our data provides the evidence for a bright hot spot in the system. The orbital period derived by us is not significantly different from the value reported by Penning et al., (1984) value. Fourier analysis of the data did not reveal any short-term periodicities in the system.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.ispartofseriesNATO Advanced Science Institutes (ASI) Series C: Mathematical and Physical Sciences;Vol. 403-
dc.rights© Kluwer Academic Publishers-
dc.subjectPhotometricen
dc.subjectPhotometric Observationsen
dc.subjectCataclysmic Variableen
dc.subjectPG 1012-029en
dc.titleFurther photometric observations of the cataclysmic variable PG 1012-029en
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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