The XRISM observatory has achieved a groundbreaking observation, documenting a stellar wind originating from a massive star being actively absorbed by its smaller, dense companion. This unprecedented detection represents direct evidence of this interaction occurring in real time. Scientists utilized data collected by the Japan-led mission to identify the powerful X-ray flares emanating from the system. These flares are now understood to be fueled directly by the captured stellar wind impacting the compact object. Researchers believe this discovery significantly advances our understanding of accretion processes and their role in generating intense radiation within binary systems across the cosmos.
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This PlaneNews briefing summarizes reporting originally published by www.nasa.gov.
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