Using NuSTAR and XMM-Newton satellites, astronomers from New York University (NYU) Abu Dhabi have observed a pulsar known as PSR J1930+1852 and its pulsar wind nebula (PWN). Results of the observational campaign, published in The Astrophysical Journal, yield more insights into the PWN and the pulsar that powers it.



Summary

NYU Abu Dhabi astronomers used NuSTAR and XMM-Newton satellites to study the pulsar PSR J1930+1852 and its surrounding pulsar wind nebula (PWN). Their research, published in The Astrophysical Journal, provides new observations and insights into the characteristics of both the PWN and the pulsar. By analyzing X-ray emissions, the study sheds light on the behavior and properties of these celestial objects, contributing to a better understanding of pulsars and their influence on their surrounding environment.

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