Volume 559, November 2013
|Number of page(s)||17|
|Section||Stellar structure and evolution|
|Published online||28 November 2013|
Best fit from PoWR modeling (thick red solid lines) to the observed HD 66811 spectra (thin blue solid lines), together with the calculated P v line profile from 3D Monte-Carlo code (black dotted line). Blue labels with numbers in the upper panels are UBVJHK magnitudes.
|Open with DEXTER|
© ESO, 2013
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