http://arxiv.org/abs/1711.02517
We report preliminary results of the analysis of the proper motion of the bright radio pulsar \b1727. 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.
P. Shternin, M. Yu, A. Shibanov, et. al.
Wed, 8 Nov 17
38/84
Comments: 5 pages; 2 figures; accepted for publication in Proceedings of PNS-2017 conference, Saint Petersburg, July 10-14, 2017