XRISM catches neutron star feeding on blue hypergiant's stellar wind
Astronomers using Japan's XRISM X-ray observatory have directly observed a blue hypergiant's stellar wind being captured by its compact companion, a superdense neutron star. This captured material powers the system's strong X-ray flares.
- Observations made with Japan-led XRISM X-ray observatory
- First direct view of a neutron star capturing stellar wind
- Hypergiant's outflow powers the system's X-ray flares
- Work is part of NASA's exploration of the extreme universe
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