pith. machine review for the scientific record. sign in

arxiv: 1612.02563 · v1 · pith:J2OCSUOInew · submitted 2016-12-08 · 🌌 astro-ph.HE

Pulse profiles and timing of PSR J1757-2421

classification 🌌 astro-ph.HE
keywords frequencylargeprofiletimingb1754glitchincreasej1757
0
0 comments X
read the original abstract

Pulse arrival time measurements over fourteen years with the Nanshan 25-m and Parkes 64-m radio telescopes have been used to determine the average profile and timing properties for PSR J1757$-$2421 (B1754$-$24). Analysis of the radio profile data shows a large variation of spectral index across the profile and an unusual increase in component separation with increasing frequency. The timing observations show that PSR B1754$-$24 underwent a large glitch with a fractional increase in spin frequency of $\Delta\nu_{\rm g}/\nu\sim 7.8\times10^{-6}$ in May 2011. At the time of the glitch there was a large permanent jump in the rotational frequency accompanied by two exponential recovery terms with timescales of 15(6) and 97(15) days, respectively.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.