Systemic recoil velocity distribution of field millisecond pulsar systems: Implications for neutron star retention in star clusters

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Table 1

Global magnitudes of the Galactic heights and the transverse peculiar velocities of the binary and the solitary millisecond pulsars.

MSPs	\|v_l\| (km s⁻¹)	\|v_b\| (km s⁻¹)	\|z\|(kpc)
Binary	$44_{- 31}^{+ 85}$ $44_{-31}^{+85}$	$34_{- 24}^{+ 56}$ $34_{-24}^{+56}$	$0 . 46_{- 0.30}^{+ 0.51}$ $0.46_{-0.30}^{+0.51}$
Solitary	$40_{- 26}^{+ 69}$ $40_{-26}^{+69}$	$17_{- 13}^{+ 26}$ $17_{-13}^{+26}$	$0 . 13_{- 0.08}^{+ 0.33}$ $0.13_{-0.08}^{+0.33}$

Notes. The lower bound, estimate, and the upper bound corresponds, respectively, to the 16th, the 50th, and the 84th percentile of each of the |v_l|,|v_b|, and |z| chains.

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