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 composite SNRs residing in the Milky Way galaxy.
![](https://3c1703fe8d.site.internapcdn.net/newman/csz/news/tmb/2019/2-astronomerst.jpg)
Source:
https://phys.org/news/2019-06-astronomers-closer-emission-supernova-remnant.html