PSR 1758 - 24 and G5.4 - 1.2, a remarkable pulsar-supernova remnant association

Details PSR 1758 - 24 and G5.4 - 1.2, a remarkable pulsar-supernova remnant association PSR 1758 - 24 and G5.4 - 1.2, a remarkable pulsar-supernova remnant association

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.253p...7m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 253, Nov. 1, 1991, p. 7P-10P. Research supported by CNR

Astronomy and Astrophysics

Astronomy

55

Pulsars, Stellar Evolution, Supernova Remnants, Radio Telescopes, Stellar Envelopes, Stellar Magnetic Fields, Very Large Array (Vla)

Scientific paper

Timing observations made over an 18-month period using the Parkes radiotelescope show that the pulsar PSR 1758 - 24 is young and is located at the extreme western edge of the compact nebula G5.27 - 0.90 which is associated with the supernova remnant G5.4 - 1.2. These results confirm the association of this pulsar with the supernova remnant. They also imply that the pulsar was born with such a high velocity that it has overtaken the supernova remnant shell and now lies outside the shell.

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