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Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1

E. Giacani·N. Loiseau·G. Dubner·M. J. S. Smith
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Abstract

We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1 belongs to the thermal composite morphological class. Small scale structures in radio and X-ray emission are not always correlated and are different for the different X-rays bands examined. The distance to G352.7-0.1 can be constrained between 6.6 and 8.4 kpc. The study of the HI suggests that G352.7-0.1 is located within a cavity probably created by the stellar wind of the precursor star.

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E. Giacani, N. Loiseau, G. Dubner, M. J. S. Smith. 2005-11-16. Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1. https://arxiv.org/abs/astro-ph/0511477

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