Astronomers from the California Institute of Technology (Caltech) and elsewhere have observed an ultraluminous X-ray source known as NGC 925 ULX-3 using NASA’s Swift and NuSTAR spacecraft, as well as ESA’s XMM-Newton satellite. Results of this observational campaign, published June 16 on arXiv.org, deliver important insights into variability behavior of this source.
Click here for original story, Research investigates variability of the ultraluminous X-ray source NGC 925 ULX-3
Source: Phys.org