Observations of Optical Emission from X-Per and SCO X-1

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4139

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DC Field	Value	Language
dc.contributor.author	Sharma, P. D	-
dc.contributor.author	Nagaraja, V. B	-
dc.contributor.author	Marar, K. T. M	-
dc.contributor.author	Bhattacharyya, J. C	-
dc.contributor.author	Mohin, S	-
dc.date.accessioned	2008-12-19T10:48:45Z	-
dc.date.available	2008-12-19T10:48:45Z	-
dc.date.issued	1981	-
dc.identifier.citation	Proceedings of the 17th International Cosmic Ray Conference, held in Paris, France. Vol. 9. pp. 13 - 16	en
dc.identifier.uri	http://hdl.handle.net/2248/4139	-
dc.description.abstract	High speed photometric observations of X-per, and SCO X-1 have been carried out during 1979-80 with the 102cm and 33cm telescope at the Kavalur observatory. Results from some of these observations are presented in this paper. Data on long term intensity variations at a level of ▲m = ± 0.1 and fast flickering in X-per are presented and discussed.	en
dc.language.iso	en	en
dc.publisher	IUPAP	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981ICRC....9...13S	en
dc.title	Observations of Optical Emission from X-Per and SCO X-1	en
dc.type	Article	en
Appears in Collections:	IIAP Publications J.C.Bhattacharyya (1982 - 1990)

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