Proper motion of the radio pulsar B1727-47 and its association with the supernova remnant RCW 114

Abstract

We report preliminary results of the analysis of the proper motion of the bright radio pulsar B1727$-$47. Using archival Parkes timing data, as well as original and archival ATCA interferometry observations, we, for the first time, constrain the pulsar proper motion at the level of 148$\pm$11 mas yr${}^{-1}$. The backward extrapolation of the proper motion vector to the pulsar birth epoch points at the center of the Galactic supernova remnant RCW 114 suggesting the genuine association between the two objects. We discuss the implications of the association and argue that the distance to the system is less than $1$ kpc. This value is at least two times lower than the dispersion measure distance estimates. This suggests that the existing Galaxy electron density models are incomplete in the direction to the pulsar.

arXiv comment5 pages; 2 figures; Proceedings of the Physics of Neutron Stars - 2017. 50 years after, Saint Petersburg, July 10-14, 2017. In ver. 2, typos corrected

References in corpus (7)

• A statistical study of 233 pulsar proper motions
• TEMPO2, a new pulsar timing package. I: Overview
• A New Electron Density Model for Estimation of Pulsar and FRB Distances
• Detection of 107 glitches in 36 southern pulsars
• TempoNest: A Bayesian approach to pulsar timing analysis
• Glitches in Southern Pulsars
• C IV Emission-line Detection of the Supernova Remnant RCW 114

Cited by in corpus (2)

• Searching a Thousand Radio Pulsars for Gamma-ray Emission
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches