Groups of space velocities in the reactive model of pulsar acceleration

Details Groups of space velocities in the reactive model of pulsar acceleration Groups of space velocities in the reactive model of pulsar acceleration

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998astl...24..222p&link_type=abstract

Astronomy Letters, Volume 24, Issue 2, March 1998, pp.222-227; Pis'ma v Astronomicheskii Zhurnal, Vol. 24, p. 268

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The previously proposed V_t ~ sin test makes it possible to estimate the space velocities of pulsars. Thirty-seven classical pulsars with errors of the transverse velocities below +/- 0.5 V_t were selected. Three pulsar groups were identified: with small, medium, and large space velocities. The differences between these groups can be traced in some of the physical parameters of pulsars.

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