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

D. A. Frall; S. R. Kulkarni; G. Vasisht

doi:10.1038/365136a0

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

Journal article

Peer reviewed

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

D. A. Frall, S. R. Kulkarni and G. Vasisht

Nature (London), Vol.365(6442), pp.136-138

09/09/1993

DOI: https://doi.org/10.1038/365136a0

Abstract

Astrophysics

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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Title: Identification of PSR1758-23 as a runaway pulsar from the supernova remnant W28
Creators - without role: D. A. Frall - National Radio Astronomy Observatory
S. R. Kulkarni - California Institute of Technology
G. Vasisht - California Institute of Technology
Publication Details: Nature (London), Vol.365(6442), pp.136-138
Identifiers: 9941084108331
Academic Unit: King Abdullah University of Science & Technology
Language: English
Resource Type: Journal article