Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-11-21
Astronomy and Astrophysics
Astrophysics
4 pages, 1 figure. To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M.
Scientific paper
Pulsars are rotating neutron stars, sweeping the emission regions from the magnetic poles across our line of sight. Isolated neutron stars lose angular momentum through dipole radiation and (possibly) particle winds, hence they slow down extremely steadily, making them amongst the most reliable timing sources available. However, it is well known that younger pulsars can suffer glitches, when they suddenly deviate from their stable rotation period. On 2000 January 16 (MJD 51559) the rate of pulsation from the Vela pulsar (B0833-45) showed such a fractional period change of 3.1 x 10^{-6}, the largest recorded for this pulsar. The glitch was detected and reported by the Hobart radio telescope. The speedy announcement allowed the X-ray telescope, Chandra, and others, to make Target of Opportunity observations. The data placed an upper limit of 40 seconds for the transition time from the orginal to the new period. Four relaxation timescales are found, which are believed to be due to the transfer of inertia through the internal structure. One is very short, about 60 seconds; the others have been previously reported and are 0.56, 3.33 and 19.1 days in length.
Dodson Richard
Lewis Dean R.
McCulloch Peter M.
No associations
LandOfFree
High time resolution observations of a Vela glitch 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 High time resolution observations of a Vela glitch, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High time resolution observations of a Vela glitch will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-340925