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XRISM measured gas plunging toward pulsar GX 301−2 at 540,000 km/h as it crossed Wray 977’s stellar wind—and found evidence that its turbulent disk breaks apart before rebuilding in the opposite direction.
XRISM's iron-line spectrum directly measured plasma falling onto GX 301−2, while the disk-breakup and reversal sequence remains a model supported by spectra and Fermi timing. The post XRISM measured gas plunging toward pulsar GX 301−2 at 540,000 km/h as it crossed Wray 977’s stellar wind—and found evidence that its turbulent disk breaks apart before rebuilding in the opposite direction. appeared first on Space Daily .
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