Stellar X-rays and magnetic activity in 3D MHD coronal models

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Fig. 11

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Scaling of averages of X-ray emission ⟨L_X⟩ with 171 Å emission as observed by AIA ⟨L₁₇₁⟩ for model runs listed in Table 1. The bars represent the standard deviation of L_X in time. The red line is a power-law fit to the data; see Sect. 6.6.

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