Fig. 14.
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Relationships between flare energy and duration in stars of different spectral type. Panel (a) shows the whole of our sample; (b) A-type stars; (c) F-type stars; (d) G-type stars; (e) K-type stars; (f) M-type stars; (g) all main sequence stars; and (h) all giants (subgiants and red giants). Values in parentheses are the corresponding number of flare events.
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