arXiv · 1106.5645
Pulse profile stability of the Crab pulsar
Abstract
We present an X-ray timing analysis of the Crab pulsar, PSR B0531+21, using the archival RXTE data. We have investigated the stability of the Crab pulse profile, in soft (2-20 keV) and hard (30-100 keV) X-ray energies, over the last decade of RXTE operation. The analysis includes measurement of the separation between the two pulse peaks; and intensity and the widths of the two peaks. We did not find any significant time dependency in the pulse shape. The two peaks are stable in phase, intensity and widths, for the last ten years. The first pulse is relatively stronger at soft X-rays. The first pulse peak is narrower than the second peak, in both, soft- and hard X-ray energies. Both the peaks show a slow rise and a steeper fall. The ratio of the pulsed photons in the two peaks is also constant in time.
Explore related subjects
Keep this discovery
Chetana Jain, Biswajit Paul. 2011-06-28. Pulse profile stability of the Crab pulsar. https://doi.org/10.1088/1674-4527/11/10/002
Cite the original work for its findings. Save a collection to share your selection of sources.