Evidence against the association of PSR B1706-44 with SNR G343.1-2.3.

Details Evidence against the association of PSR B1706-44 with SNR G343.1-2.3. Evidence against the association of PSR B1706-44 with SNR G343.1-2.3.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...306l..49n&link_type=abstract

Astronomy and Astrophysics, v.306, p.L49

Astronomy and Astrophysics

Astrophysics

26

Pulsars: Individual: Psr B1706-44, Stars: Neutron, Stars: Kinematics, Ism: Individual: Snr G343.1-2.3, Ism: Supernova Remnants, Ism: Structure

Scientific paper

An association between the supernova remnant SNR G343.1-2.3 and the pulsar PSR B1706-44 would imply a pulsar velocity greater than 1000km/s. Observations of the pulsar scintillation made with the Parkes radio telescope at 20 and 70cm indicate a velocity less than 50km/s. This fact, coupled with statistical arguments and the morphology of both the SNR and the pulsar plerion, shows that the association between the two objects is merely geometric projection.

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