The X-ray spectrum of S1 in SNR CTB 37B is better described by a broken power law with a break near 5.6 keV than by a single power law, and a non-thermal bremsstrahlung model with young electrons can match it.
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Investigation of the non-thermal X-ray emission from the supernova remnant CTB 37B hosting the magnetar CXOU J171405.7$-$381031
The X-ray spectrum of S1 in SNR CTB 37B is better described by a broken power law with a break near 5.6 keV than by a single power law, and a non-thermal bremsstrahlung model with young electrons can match it.