Query : 2001A&A...369..174G

2001A&A...369..174G - Astronomy and Astrophysics, volume 369, 174-177 (2001/4-1)

On the velocity of the Vela pulsar.


Abstract (from CDS):

It is shown that if the shell of the Vela supernova remnant is responsible for nearly all the scattering of the Vela pulsar, then the scintillation and proper motion velocities of the pulsar can only be reconciled with each other in the case of nonzero transverse velocity of the scattering material. A possible origin of large-scale transverse motions in the shell of the Vela supernova remnant is discussed.

Abstract Copyright:

Journal keyword(s): pulsars: individual: Vela - ISM: individual objects: Vela supernova remnant - scattering

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
1 NAME GUM Nebula ISM 07 43 -42.1           ~ 417 1
2 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1209 2
3 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2273 1

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