Study of X-ray pulsars Cep X-4 and 4U 1907+09

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4991

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DC Field	Value	Language
dc.contributor.author	Agrawal, P.C.	-
dc.contributor.author	Mukerjee, K.	-
dc.contributor.author	Paul, Biswajit	-
dc.contributor.author	Rao, A.R.	-
dc.contributor.author	Seetha, S.	-
dc.contributor.author	Kasturirangan, K.	-
dc.date.accessioned	2012-07-19T08:52:33Z	-
dc.date.available	2012-07-19T08:52:33Z	-
dc.date.issued	1999	-
dc.identifier.citation	Astronomische Nachrichten, 1999, Vol. 320, p346	en
dc.identifier.issn	0004-6337	-
dc.identifier.issn	1521-3994 (Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/4991	-
dc.description	Restricted Access	en
dc.description.abstract	The X-ray pulsars Cep X-4 and 4U 1907+09 were observed with the pointed mode proportional counters(PPCs) of Indian X-ray Astronomy Experiment(IXAE) on IRS-P3 satellite. Detailed studies of pulse profile of Cep X-4 revealed an inter-pulse dominated double-pulse profile. In the case of pulsar 4U 1907+09, the pulse period measurements indicate spindown of the pulsar with P=+0.21 s yr−1 using the IXAE observations.	en
dc.language.iso	en	en
dc.publisher	Wiley-VCH	en
dc.rights	1999 Wily-VCH	en
dc.title	Study of X-ray pulsars Cep X-4 and 4U 1907+09	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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