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Matteo Cantiello edited intro_b.tex
about 11 years ago
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...
produced by these near surface convection zones. In particular, we examine
whether a link exists between these convective regions and
observable small scale velocity fields at the stellar surface
and in the stellar
wind, ``microturbulence". wind,"microturbulence".
A similar idea has been used to explain microturbulence
in low mass stars \cite{Edm78}, in which deeper
envelope convection zones reach the photosphere.