Solar Mn I 5432/5395 Åline formation explained
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20010223/pdf
Reference15 articles.
1. Spherically Symmetric Model Atmospheres for Low‐Mass Pre–Main‐Sequence Stars with Effective Temperatures between 2000 and 6800 K
2. Analysis of Mn I lines in the solar spectrum using accurate oscillator strengths
3. Manganese and carbon lines as temperature indicators
4. TheNextGenModel Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 K
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