Empirical investigation on the impact of hydrogen collisions for the formation of C i 1.07 μm lines based on the solar center-to-limb variation
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/66/2/32/4358520/psu001.pdf
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3. Does the radial–tangential macroturbulence model adequately describe the spectral line broadening of solar-type stars?*;Publications of the Astronomical Society of Japan;2017-04-13
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