Image of a satellite that reveals the resulting emissions of the remains of "Supernova" close

science and technology

By analyzing the data from the Suzaku X-ray satellite, astronomers have been able to come up with important information regarding the thermal and non-thermal emissions of the supernova MSH 15-56, the supernova or so-called velocity is the star burst.

According to the site "phys", the results of the study conducted through the satellite data provide an illustrated picture that can be useful in enhancing knowledge about the remains of these SNRs found in the Milky Way galaxy.

The remains of the supernova

MSH 15-56 is about 13400 light years away, and is a remnant of a SNR supernova. Given that x-ray observations have the ability to detect detailed information about complex SNRs, a team of astronomers in the Netherlands decided to conduct a study on MSH 15 Using data provided by the Suzaku X-ray satellite.

Data analysis allowed them to investigate the nature of emissions, and thermal and non-thermal emission from the southwestern margin of MSH 15-56 was found during satellite data analysis.