Identification of PSR1758-23 as a runaway pulsar from the supernova remnant W28

Details Identification of PSR1758-23 as a runaway pulsar from the supernova remnant W28 Identification of PSR1758-23 as a runaway pulsar from the supernova remnant W28

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993natur.365..136f&link_type=abstract

Nature (ISSN 0028-0836), vol. 365, no. 6442, p. 136-138.

Astronomy and Astrophysics

Astronomy

77

Extragalactic Radio Sources, Pulsars, Supernova Remnants, Very Large Array (Vla), Astronomical Photography, H Ii Regions, Interstellar Matter, Linear Polarization, Plasma Density

Scientific paper

New observations are presented which indicate that the large dispersion
and scattering of the pulses from PSR1758-23 are caused by a dense
screen of ionized material located along the line of sight. This
reconciles the distances to the pulsar with that to SNR W28.

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