Fig. 19.
Evolution of the flare observed in HII 405. Left panel: merged MOS+PN light curve in broad, soft, and hard energy bands (dots) superimposed on the K2 light curve (green asterisks). The horizontal green lines mark the defined blocks and the vertical dashed areas correspond to the bad time intervals (Sect. 3.2). Central panels: time evolution of plasma temperature and emission measure, right panel: evolution of the flare in the log(T) vs. 0.5 × log(EM) plane. The red dashed line marks the slope of the cooling phase.
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