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Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test of the accuracy of the solar iron abundance, which sets the… Click to show full abstract
Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test of the accuracy of the solar iron abundance, which sets the absolute zero-point of all stellar m ...
Keywords:
non lte;
line formation;
lte line;
formation late;
late type;
type stars
Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2017
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Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2017
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!