Suzaku XIS1 image of the SW rim of MSH 15−56 in the 0.3−10 keV energy band. The SW region is shown by the blue elliptical area. The background region is indicated by the dashed box, and the white box represents the FoV of XIS1. Credit: Cesur et al., 2019. By analyzing archival data from the Suzaku X-ray satellite, astronomers have learned important information regarding thermal and non-thermal emission from the composite supernova remnant (SNR) designated MSH 15-56. Results of the study, available in a paper published May 29 on arXiv.org, could be helpful in advancing the knowledge about co...
https://phys.org/news/2019-06-astronomers-closer-emission-supernova-remnant.html
2019-06-05 13:35:51Z
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