Flare peak intensity and duration distributions in the M87 nucleus and HST-1 knot follow power laws with consistent indices, suggesting a common magnetic reconnection origin.
@doi [ ] 10.1007/s11207-011-9755-0, http://adsabs.harvard.edu/abs/2011SoPh..274...99A 274
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Statistical analysis on X-ray flares from the nucleus and HST-1 knot in the M87 jet
Flare peak intensity and duration distributions in the M87 nucleus and HST-1 knot follow power laws with consistent indices, suggesting a common magnetic reconnection origin.