Atmospheric Models of Flare Stars: The Quiescent State of Ad Leo
P. Mauas, A. Falchi
Abstract
We compute a semi-empirical atmospheric model for the dMe star AD Leo, which constitutes the first model computed to match the continuum observations, as well as a wide set of chromospheric spectral lines. We find good agreement between the computed and observed spectral features, with the exception of the Ca II K line.
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