DEEP MORPHOLOGICAL and SPECTRAL STUDY of the SNR RCW 86 with FERMI-LAT
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Abstract
RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at
several wavelengths and is thought to be an efficient cosmic-ray (CR)
accelerator. Earlier \textit{Fermi} Large Area Telescope results reported the
detection of
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1538-4357