New VLA observations of the SNR Puppis A: the radio properties and the correlatoin withe the X-ray emission
arXiv:astro-ph/0607200 · doi:10.1051/0004-6361:20065061
Abstract
In this paper we report on a new study of the SNR Puppis A based on VLA observations at 1425 MHz; the improvement represents a factor of two in angular resolution and almost ten times in sensitivity compared to the best previous image of Puppis A. This new image is used to compare with re-processed 327 MHz data and ROSAT and Chandra images to investigate morphological and spectral characteristics.
14 pages, 9 figures, accepted for publication in A & A