Radio observations of G320.4-01.2 and PSR B1509-58

Details Radio observations of G320.4-01.2 and PSR B1509-58 Radio observations of G320.4-01.2 and PSR B1509-58

1998-10-29

arxiv.org/abs/astro-ph/9810472v1

Astronomy and Astrophysics

Astrophysics

6 pages, 3 embedded PS figures. Presented at the workshop "The Relationship between Neutron Stars and Supernova Remnants", and

Scientific paper

G320.4-01.2 is a complex radio and X-ray source, coinciding on the sky with the young energetic pulsar B1509-58. A young pulsar embedded in a SNR would seem to accord with expectations, but previous observations suggest that all may not be what it seems. Controversy persists over whether the pulsar and the SNR are associated, and as to what causes the remnant's unusual appearance. To answer these questions, we have undertaken a set of high-resolution radio observations of the system. We present the results of this study, which provide new evidence that PSR B1509-58 is associated with and is interacting with G320.4-01.2.

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