Swift monitoring reveals a factor-of-two X-ray flare from the AGN in NGC 1275 that is inconsistent with a tidal disruption event, with a radio flare following about 300 days later.
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X-ray Flaring and Variability in NGC 1275, the Heart of the Perseus Cluster
Swift monitoring reveals a factor-of-two X-ray flare from the AGN in NGC 1275 that is inconsistent with a tidal disruption event, with a radio flare following about 300 days later.