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

Douglas C. -J. Bock·V. V. Gvaramadze
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Abstract

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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Douglas C. -J. Bock, V. V. Gvaramadze. 2001-11-22. Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3. https://arxiv.org/abs/astro-ph/0111430

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