Atmospheric Models of Flare Stars: The Quiescent State of Ad Leo
Abstract
Description
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.
13 pages, 10 figures available upon request, tex dialect, ARCETRI-PR-93-29
13 pages, 10 figures available upon request, tex dialect, ARCETRI-PR-93-29