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Retrieved on: 2024-09-27 14:30:03
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Summary
This article explains the cataclysmic eruption of the hydrogen-fueled T Coronae Borealis, a binary star where a white dwarf accretes material from a red giant. Key concepts include stellar evolution and hydrogen fuel, linked through terms like cataclysmic variable stars and novas, visible in constellations such as Corona Borealis.
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