Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3

Details Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3 Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3

2001-11-22

arxiv.org/abs/astro-ph/0111430v1

ASP Conf.Ser. 271 (2002) 49

Astronomy and Astrophysics

Astrophysics

(4 pages) To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler

Scientific paper

We present some arguments in support of the association of the pulsar PSR B1706-44 with the supernova remnant G343.1-2.3, based on the idea that these objects could be the result of a supernova explosion within a mushroom-like cavity (created by the supernova progenitor wind breaking out of the parent molecular cloud). We suggest that in addition to the known bright "half" of G343.1-2.3 there should exist a more extended and weaker component, such that the actual shape of G343.1-2.3 is similar to that of the well-known SNR VRO 42.05.01. We have found such a component in archival radio data.

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