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A statistical study of 233 pulsar proper motions

TLDR
In this article, a catalogue of 233 pulsars with proper motion measurements is presented and analyzed, which contains a wide variety of pulsars including recycled objects and those associated with globular clusters or supernova remnants.
Abstract
We present and analyse a catalogue of 233 pulsars with proper motion measurements. The sample contains a wide variety of pulsars including recycled objects and those associated with globular clusters or supernova remnants. After taking the most precise proper motions for those pulsars for which multiple measurements are available, the majority of the proper motions (58 per cent) are derived from pulsar timing methods, 41 per cent using interferometers and the remaining 1 per cent using optical telescopes. Many of the one-dimensional (1D) and two-dimensional (2D) speeds (referring to speeds measured in one coordinate only and the magnitudes of the transverse velocities, respectively) derived from these measurements are somewhat lower than earlier estimates because of the use of the most recent electron density model in determining pulsar distances. The mean 1D speeds for the normal and recycled pulsars are 152(10) and 54(6) km s −1 , respectively. The corresponding mean 2D speeds are 246(22) and 87(13) km s −1 . PSRs B2011+38 and B2224+64 have the highest inferred 2D speeds of ∼1600 km s −1 .W estudy the mean speeds for different subsamples and find that, in general, they agree with previous results. Applying a novel deconvolution technique to the sample of 73 pulsars with characteristic ages less than 3 Myr, we find the mean threedimensional (3D) pulsar birth velocity to be 400(40) km s −1 . The distribution of velocities is well described by a Maxwellian distribution with 1D rms σ = 265 km s −1 . There is no evidence for a bimodal velocity distribution. The proper motions for PSRs B1830−08 and B2334+61 are consistent with their proposed associations with the supernova remnants W41 and G114.3+0.3, respectively. Ke yw ords: stars: kinematics ‐ pulsars: general.

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Explosion Mechanisms of Core-Collapse Supernovae

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References
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Journal ArticleDOI

The Australia Telescope National Facility Pulsar Catalogue

TL;DR: A new and complete catalog of the main properties of the 1509 pulsars for which published information currently exists, which includes all spin-powered pulsars, as well as anomalous X-ray pulsars and soft gamma-ray repeaters showing coherent pulsed emission.
Journal ArticleDOI

The ATNF Pulsar Catalogue

TL;DR: In this paper, the authors search the literature to find papers announcing the discovery of pulsars or giving improved parameters for them, and then they enter these papers' data into a new pulsar catalogue that can be accessed via a web interface or from the command line (on Solaris or Linux machines).
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Pulsar distances and the galactic distribution of free electrons

TL;DR: In this paper, the authors present a quantitative model for the Galactic free electron distribution, which abandons the assumption of axisymmetry and explicitly incorporates spiral arms; their shapes and locations are derived from existing radio and optical observations of H II regions.
Journal ArticleDOI

Local stellar kinematics from Hipparcos data

TL;DR: From the parallaxes and proper motions of a kinematically unbiased subsample of the Hipparcos Catalogue, it is re-determined as a function of colour the kinematics of main-sequence stars that spiral arms are responsible for the non-axisymmetry and that R0/Rd ≃ 3 to 3, where Rd is the scalelength of the disc.
Journal ArticleDOI

Review of galactic constants

TL;DR: The authors adopte les deux constantes R 0 =8,5 kpc and O 0 =220 kms −1, which are the deux constants used in this paper.
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