A supernova remnant associated with the young gamma-ray pulsar PSR1706-44

Details A supernova remnant associated with the young gamma-ray pulsar PSR1706-44 A supernova remnant associated with the young gamma-ray pulsar PSR1706-44

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993natur.361..516m&link_type=abstract

Nature (ISSN 0028-0836), vol. 361, no. 6412, p. 516-518.

Physics

53

Gamma Rays, Pulsars, Stellar Evolution, Supernova Remnants, Gamma Ray Telescopes, Point Sources, Radio Stars, Stellar Structure, X Ray Stars

Scientific paper

The field around the young gamma-ray pulsar PSR1706-44 has been mapped
with a resolution of 44 arcsec, and a shell-type SNR has been identified
at a distance of about 3 kpc. This distance is consistent with that
deduced for the pulsar. The pulsar is seen as a slightly variable point
source located in an enhanced knot on the arc of the SNR shell.

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