A Systematic Study of the Thermal and Nonthermal Emission in the Supernova Remnant RCW 86 with Suzaku
Yoshio Tsubone (1), Makoto Sawada (1), Aya Bamba (1,2,3), Satoru, Katsuda (4), Jacco Vink (5) ((1) Aoyama Gakuin U., (2) U. of Tokyo, (3), RESCEU, U. of Tokyo, (4) Chuo U., (5) GRAPPA, U. of Amsterdam)

TL;DR
This study uses Suzaku to analyze the thermal and nonthermal X-ray emissions in supernova remnant RCW 86, revealing how environmental factors influence particle acceleration and maximum energy of electrons.
Contribution
It provides spatially resolved spectroscopy of RCW 86, linking shock environment to acceleration efficiency and maximum electron energy, a novel insight into SNR physics.
Findings
Photon index decreases with lower emission measure of shocked ISM.
Maximum electron energy is higher in low-density, high-shock-speed regions.
Spectral data fit with combined thermal plasma and synchrotron models.
Abstract
Diffusive shock acceleration by the shockwaves in supernova remnants (SNRs) is widely accepted as the dominant source for Galactic cosmic rays. However, it is unknown what determines the maximum energy of accelerated particles. The surrounding environment could be one of the key parameters. The SNR RCW 86 shows both thermal and non-thermal X-ray emission with different spatial morphologies. These emission originate from the shock-heated plasma and accelerated electrons respectively, and their intensities reflect their density distributions. Thus, the remnant provides a suitable laboratory to test possible association between the acceleration efficiency and the environment. In this paper, we present results of spatially resolved spectroscopy of the entire remnant with Suzaku. The spacially-resolved spectra are well reproduced with a combination of a power-law for synchrotron emission and…
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