Pulse profiles and timing of PSR J17572421
arXiv:1612.02563 · doi:10.1093/mnras/stw3203
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 J17572421 (B175424). 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 B175424 underwent a large glitch with a fractional increase in spin frequency of 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.
9 pages, 8 figures, 5 tables, Accepted for publication in MNRAS
References in corpus (13)
- TEMPO2, a new pulsar timing package. I: Overview
- PSRCHIVE and PSRFITS An Open Approach to Radio Pulsar Data Storage and Analysis
- Tempo2, a new pulsar timing package. II: The timing model and precision estimates
- Switched magnetospheric regulation of pulsar spin-down
- Neutron conduction in the inner crust of a neutron star in the framework of the band theory of solids
- Detection of 107 glitches in 36 southern pulsars
- Avalanche dynamics of radio pulsar glitches
- Pulsar Timing for the Fermi Gamma-ray Space Telescope
- A hydrodynamical trigger mechanism for pulsar glitches
- A Fan Beam Model for Radio Pulsars. I. Observational Evidence
- Two types of glitches in a solid quark star model
- A strong correlation in radio pulsars with implications for torque variations
- Frequency dependence of pulse width for 150 radio normal pulsars