Does the radial–tangential macroturbulence model adequately describe the spectral line broadening of solar-type stars?*
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/69/3/46/17668567/psx022.pdf
Reference43 articles.
1. Nonthermal broadening in the solar photosphere derived from widths of weak absorption features in the CA II H and K wings
2. A measurement of the non-thermal velocity in the low chromosphere
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