Millisecond pulsar velocities

被引:90
作者
Toscano, M [1 ]
Sandhu, JS
Bailes, M
Manchester, RN
Britton, MC
Kulkarni, SR
Anderson, SB
Stappers, BW
机构
[1] Univ Melbourne, Dept Phys, Parkville, Vic 3052, Australia
[2] Swinburne Univ Technol, Hawthorn, Vic 3122, Australia
[3] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[4] CSIRO, Australia Telescope Natl Facil, Epping, NSW 2121, Australia
[5] Australian Natl Univ, Mt Stromlo & Siding Spring Observ, Weston Creek, ACT 2611, Australia
关键词
stars : kinematics; pulsars : general;
D O I
10.1046/j.1365-8711.1999.02685.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present improved timing parameters for 13 millisecond pulsars (MSPs), including nine new proper motion measurements. These new proper motions bring to 23 the number of MSPs with measured transverse velocities. In light of these new results we present and compare the kinematic properties of MSPs with those of ordinary pulsars, The mean transverse velocity of MSPs was found to be 85 +/- 13 km s(-1), a value consistent with most models for the origin and evolution of MSP's and approximately a factor of 4 lower than that of ordinary pulsars. We also find that, in contrast to young ordinary pulsars, the vast majority of which are moving away from the Galactic plane, almost half of the MSPs are moving towards the plane. This near-isotropy would be expected of a population that has reached dynamic equilibrium. Accurate measurements of MSP velocities have allowed us to correct their measured spin-down rates for Doppler acceleration effects, and thereby derive their intrinsic magnetic field strengths and characteristic ages. We find that close to half of our sample of MSPs have a characteristic age comparable to or greater than the age of the Galactic disc.
引用
收藏
页码:925 / 933
页数:9
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