Atmospheric Models of Flare Stars: The Quiescent State of Ad Leo
classification
🌌 astro-ph
keywords
atmosphericcomputedmodelspectralagreementchromosphericcomputeconstitutes
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.