Hard X-ray Contribution in AU Mic Flares and Its Minor Role in Atmospheric Escape

[2508.15107] Hard X-ray Contribution in AU Mic Flares and Its Minor Role in Atmospheric Escape Skip to main content We gratefully acknowledge support from the Simons Foundation, member institutions , and all contributors.
Overall, the flares are thermally dominated, nonthermal electrons can power chromospheric heating episodically, but HXR-induced escape appears to be marginal for the long-term atmospheric evolution of AU Mic’s planets.
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