Glitches from the Young Pulsar J1833-1034

Details Glitches from the Young Pulsar J1833-1034 Glitches from the Young Pulsar J1833-1034

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..407..299r&link_type=abstract

The Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8-12 December 2008, at Nati

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present preliminary results from out timing study of the young pulsar, PSR J1833-1034, in the supernova remnant G21.5-0.9. From the detailed behaviour of the timing residuals, we are able to infer the occurrence of as many as three glitches over a span of 3.5 years. The fractional change of the rotational frequency during these glitches is found to be in the range 1× 10-9 to 3×10-9. The final model fitted to the timing data yields accurate estimates for the period, its first and second derivatives, and hence a plausible value of the braking index.

Affiliated with

Also associated with

No associations

Rating

Glitches from the Young Pulsar J1833-1034 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 Glitches from the Young Pulsar J1833-1034, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Glitches from the Young Pulsar J1833-1034 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-834204