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

dc.contributor.authorAgrawal, P C
dc.contributor.authorMukerjee, K
dc.contributor.authorPaul, Biswajit
dc.contributor.authorRao, A R
dc.contributor.authorSeetha, S
dc.contributor.authorKasturirangan, K
dc.date.accessioned2012-07-19T08:52:33Z
dc.date.available2012-07-19T08:52:33Z
dc.date.issued1999
dc.descriptionRestricted Accessen
dc.description.abstractThe 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.identifier.citationAstronomische Nachrichten, 1999, Vol. 320, p346en
dc.identifier.issn0004-6337
dc.identifier.issn1521-3994 (Online)
dc.identifier.urihttp://hdl.handle.net/2289/4991
dc.language.isoenen
dc.publisherWiley-VCHen
dc.rights1999 Wily-VCHen
dc.titleStudy of X-ray pulsars Cep X-4 and 4U 1907+09en
dc.typeArticleen

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