Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44

Details Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44 Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasb.conf...67l&link_type=abstract

"Pulsars, AXPs and SGRs observed with BeppoSAX and Other Observatories, Proceedings of the International Workshop held in Marsal

Other

Scientific paper

We present the results of long-term timing measurements of the radio pulsars PSR J0538+2817 and PSR B1853+01. The first of them is apparently associated with the well-known galactic anticenter remnant S147, but no conclusive proof of a physical connection between the two objects exists. A timing activity of PSR J0538+2817 is typical of middle-aged pulsars, but it is high enough to make the timing astrometry of this object unreliable. Radio interferometry and X-ray observations of the W44 remnant strongly suggests that PSR B1853+01 is associated with it. Here, we report a detection of three timing glitches in this source and show that its overall timing activity is comparable to that of the Crab pulsar.

Affiliated with

Also associated with

No associations

Rating

Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Timing Characteristics of Radio Pulsars in the Supernova Remnants S147 and W44 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885007