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2000A&A...358..575J - Astronomy and Astrophysics, volume 358, 575-582 (2000/6-2)
The contribution of the micro-turbulent velocity on the modelling of chromospheric lines in late type dwarfs.
JEVREMOVIC D., DOYLE J.G. and SHORT C.I.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): line: formation - line: profiles - turbulence - stars: activity - stars: chromospheres - stars: late-type
Simbad objects: 4
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