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Relativistic outflows power a quasi-periodic eruption: constraints on energetics, mass loss, and emission mechanisms
Quasi-periodic eruptions (QPEs) are recurring bursts of X-ray radiation originating from supermassive black holes (SMBHs). They are an unprecedented type of structured, high-amplitude SMBH variability, but the physical origins of their regularity, timescales, energetics, and emission are uncertain.
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