Further photometric observations of the cataclysmic variable PG 1012-029

Ashoka, B. N; Marar, T. M. K; Seetha, S; Kasturirangan, K; Rao, U. R; Bhattacharyya, J. C

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dc.contributor.author	Ashoka, B. N
dc.contributor.author	Marar, T. M. K
dc.contributor.author	Seetha, S
dc.contributor.author	Kasturirangan, K
dc.contributor.author	Rao, U. R
dc.contributor.author	Bhattacharyya, J. C
dc.date.accessioned	2009-07-11T12:41:09Z
dc.date.available	2009-07-11T12:41:09Z
dc.date.issued	1993
dc.identifier.citation	Barstow, 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 – 541	en
dc.identifier.isbn	0-7923-2332-7
dc.identifier.uri	http://hdl.handle.net/2248/4629
dc.description	Restricted Access
dc.description.abstract	We 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.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.ispartofseries	NATO Advanced Science Institutes (ASI) Series C: Mathematical and Physical Sciences;Vol. 403
dc.rights	© Kluwer Academic Publishers
dc.subject	Photometric	en
dc.subject	Photometric Observations	en
dc.subject	Cataclysmic Variable	en
dc.subject	PG 1012-029	en
dc.title	Further photometric observations of the cataclysmic variable PG 1012-029	en
dc.type	Article	en