New VLA observations of the SNR Puppis A: the radio properties and the correlatoin withe the X-ray emission

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.

arXiv comment14 pages, 9 figures, accepted for publication in A & A

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• The most complete and detailed X-ray view of the SNR Puppis A
• What planetary nebulae can tell us about jets in core collapse supernovae
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• H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A
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• High resolution CO observations towards the Bright Eastern Knot of the SNR Puppis A
• Kinematics of Supernova Remnants: Status of X-Ray Observations
• Global X-Ray Properties of the Vela and Puppis A Supernova Remnants
• Evidence for protons accelerated and escaped from the Puppis A region using \textit{Fermi}-LAT observations