Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4900
Full metadata record
DC FieldValueLanguage
dc.contributor.authorMukerjee, K.-
dc.contributor.authorAgrawal, P.C.-
dc.contributor.authorPaul, Biswajit-
dc.contributor.authorRao, A.R.-
dc.contributor.authorYadav, J.S.-
dc.contributor.authorSeetha, S.-
dc.contributor.authorKasturirangan, K.-
dc.date.accessioned2012-07-14T09:42:38Z-
dc.date.available2012-07-14T09:42:38Z-
dc.date.issued2000-06-
dc.identifier.citationBulletin of the Astronomical Society of India, Vol.28, p293-294en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2289/4900-
dc.descriptionRestricted Accessen
dc.description.abstractThe X-ray pulsars Cep X-4 and 4U 1907+09 were observed with the Indian X-ray Astronomy Experiment (IXAE). Observations of Cep-X4 were made during the declining phase of its latest 30 days outburst in 1997, July-August. The X-ray pulse profiles obtained during IXAE observations show inter-pulse dominated double-peak pulse. The second X-ray pulsar 4U 1907+09 with a period of 440s was observed in August 1996 and again in June 1998. The X-ray profile shows a double-peak pulse shape. The P obtained from these two observations indicate that the pulsar is in monotonically spin-down phase, at the rate of 0.23 s yr-1.en
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..293Men
dc.rights2000 The Astronomical Society of Indiaen
dc.subjectX-ray pulsaren
dc.subjectIXAEen
dc.titleStudy of two pulsars with the Indian X-ray Astronomy Experimenten
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2000_BASI_V28__p293.pdf
  Restricted Access
Restricted Access168.32 kBAdobe PDFView/Open Request a copy


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.