Hostname: page-component-7bb8b95d7b-5mhkq Total loading time: 0 Render date: 2024-09-11T18:18:52.297Z Has data issue: false hasContentIssue false
  • English
  • Français

Long-Term X-ray Variability of Circinus X-1 as Observed by the RXTE All Sky Monitor

Published online by Cambridge University Press:  26 May 2016

Junfeng Wang  and
W. N. Brandt
Junfeng Wang
Affiliation:
Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA
W. N. Brandt
Affiliation:
Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The luminous low mass X-ray binary Cir X-1 has been observed nearly continuously for about 5 years by the X-ray All Sky Monitor on board the RXTE satellite. We carried out a timing analysis on Cir X-1 with the RXTE data. We define the period from the X-ray data, comparing the period change over time with the best current ephemeris. with folded light curves of entire data set, characteristics of the system like long-term lightcurve changes, behavior of flares and dips and super-Eddington accretion were obtained. We also checked and identified the secondary flaring reported in radio band with X-ray data.

Type
Part 6 X-Ray Binaries
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 218 - 219
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Brandt, W. N. et al. 1996, MNRAS, 283, 1071 Google Scholar
Fender, R. P. 1997, Proceedings of the Fourth Compton Symposium, AIP Google Scholar
Shirey, R. E., Bradt, H. V., Levine, A. M., & Morgan, E. H., 1996, ApJ, 469, L21 Google Scholar