Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-26T22:20:24.975Z Has data issue: false hasContentIssue false

PSRSalsa and the bi-drifting pulsar B1839–04

Published online by Cambridge University Press:  04 June 2018

Patrick Weltevrede*
Affiliation:
Jodrell Bank Centre for Astrophysics, The University of Manchester Alan Turing Building, Manchester, M13 9PL, United Kingdom email: Patrick.Weltevrede@manchester.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

PSRSalsa is a versatile open-source pulsar data-analysis project designed to obtain a comprehensive picture of the radio properties of your pulsar of choice. Here its usefulness is demonstrated through the analysis of the radio pulsar B1839–04, thereby revealing the extremely rare phenomenon of “bi-drifting” where the drift direction of subpulses is systematically different in different pulse profile components.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Champion, D. J., et al., 2005, MNRAS, 363, 929Google Scholar
Ruderman, M. A., & Sutherland, P. G., 1975, ApJ, 196, 51Google Scholar
Weltevrede, P., 2016, A&A, 590, 109Google Scholar
Wright, G. A. E., & Weltevrede, P., 2017, MNRAS, 464, 2597Google Scholar