ARTICLE AD BOX
The star γ Cas, visible to the naked eye in the constellation Cassiopeia, has confused astronomers for decades. It produces X-rays far more intense and hotter than what scientists expect from a typical massive star. New observations using the Resolve instrument aboard Japan's XRISM space telescope now link these emissions to a white dwarf orbiting the star. This discovery also confirms a long-predicted type of binary system that had never been clearly identified. The findings, led ...

4 days ago
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