Near absence of hard X-ray pulsation from GS 1843+00 in the middle of burst phase

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DC Field	Value	Language
dc.contributor.author	Manchanda, R. K	-
dc.date.accessioned	2008-02-29T11:30:36Z	-
dc.date.available	2008-02-29T11:30:36Z	-
dc.date.issued	2000	-
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 277 - 280	en
dc.identifier.uri	http://hdl.handle.net/2248/2102	-
dc.description.abstract	Hard X-ray transient pulsar GS 1843+00 was observed in the 20-200keV region using a high sensitivity large area scintillation counter instrument during its 1997 flare on March 30. The data indicates a near absence of 29.5s pulsation in the hard X-ray energy band of 30-70 keV, even though our observations correspond near to intensity maximum in the burst phase. Along with the RXTE and Compton observatory data taken during this burst, we discuss the present results in terms of geometrical constraints and the X-ray emission mechanism.	en
dc.format.extent	614690 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..277M	en
dc.subject	X-ray pulsation	en
dc.subject	X-ray	en
dc.title	Near absence of hard X-ray pulsation from GS 1843+00 in the middle of burst phase	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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