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Meredith L. Rawls edited section_Stellar_atmosphere_models_label__.tex
over 8 years ago
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\section{Stellar atmosphere models}
\label{atmosphere}
Disentangling spectra with FDBinary \citep{ili04} is fun and easy. Some lines are good magnetic diagnostics.
We have flux ratios from $BVRI$ photometry, which is necessary to properly fit stellar atmosphere models to component spectra.