Study of two pulsars with the Indian X-ray Astronomy Experiment

dc.contributor.author	Mukerjee, K
dc.contributor.author	Agrawal, P. C
dc.contributor.author	Paul, B
dc.contributor.author	Rao, A. R
dc.contributor.author	Yadav, J. S
dc.contributor.author	Seetha, S
dc.contributor.author	Kasturirangan, K
dc.date.accessioned	2008-03-03T08:11:47Z
dc.date.available	2008-03-03T08:11:47Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 293 - 294	en
dc.identifier.uri	http://hdl.handle.net/2248/2105
dc.description.abstract	The 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.format.extent	168375 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..293M	en
dc.subject	X-ray pulsar	en
dc.subject	IXAE	en
dc.subject	Profile	en
dc.title	Study of two pulsars with the Indian X-ray Astronomy Experiment	en
dc.type	Article	en