VLBI astrometry of two millisecond pulsars

Abstract

We present astrometric results on two millisecond pulsars, PSR B1257+12 and PSR J1022+1001, as carried out through VLBI. For PSR B1257+12, a model-independent distance of $710_{-38}^{+43}$ pc and proper motion of ($\hat{I}{¼}_{\hat{\mathrm{I}}\pm }=46.44\pm 0.08$ mas/yr, $\hat{I}{¼}_{\hat{\mathrm{I}}´}=-84.87\pm 0.32$ mas/yr) were obtained from 5 epochs of VLBA and 4 epochs of EVN observations, spanning about 2 years. The two dimensional proper motion of PSR J1022+1001 ($\hat{I}{¼}_{\hat{\mathrm{I}}\pm }\sim -10.13$ mas/yr, $\hat{I}{¼}_{\hat{I}}´\sim 16.89$ mas/yr) was also estimated, using 3 epochs of EVN observations. Based on our results, the X-ray efficiency of PSR B1257+12 should be in the same range as other millisecond pulsars, and not as low as previously thought.

Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 3 pages