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Paper: |
Physical Conditions in Regions of Line Formation of Solar Type Stars |
Volume: |
472, New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-like Stars, With and Without Planets |
Page: |
187 |
Authors: |
Rodríguez-Merino, L. H.; Cardona, O.; Flores, A. |
Abstract: |
We present the physical properties of the regions in the atmospheres of solar type stars
where the atomic spectral lines are forming. We used selected spectra from ELODIE library to
measure the width of the Balmer, sodium, and magnesium lines. The results allowed us to
infer the temperature and the total particle number density of the regions where each line
is forming. The physical conditions obtained in this work were compared with the results of
stellar atmosphere models. |
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