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, Biswajit | |
| 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 | 2012-07-14T09:42:38Z | |
| dc.date.available | 2012-07-14T09:42:38Z | |
| dc.date.issued | 2000-06 | |
| dc.description | Restricted Access | en |
| 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.identifier.citation | Bulletin of the Astronomical Society of India, Vol.28, p293-294 | en |
| dc.identifier.issn | 0304-9523 | |
| dc.identifier.uri | http://hdl.handle.net/2289/4900 | |
| dc.language.iso | en | en |
| dc.publisher | The Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/2000BASI...28..293M | en |
| dc.rights | 2000 The Astronomical Society of India | en |
| dc.subject | X-ray pulsar | en |
| dc.subject | IXAE | en |
| dc.title | Study of two pulsars with the Indian X-ray Astronomy Experiment | en |
| dc.type | Article | en |