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Turbulence in Main Sequence Stars

Published online by Cambridge University Press:  12 April 2016

Thomas Gehren
Thomas Gehren*
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl, 6900 Heidelberg, Germany

Extract

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It has for long been realized that the interpretation of stellar spectral lines normally requires broadening velocities well in excess of purely thermal motions. The origin and structure of such velocity fields, which have usually been summarized as turbulence, still appear to be a subject of controversy.

Type
2. Observed Properties of Stellar Turbulence
Information
International Astronomical Union Colloquium , Volume 51: Stellar Turbulence , 1980 , pp. 103 - 112
Copyright
Copyright © Springer-Verlag 1980

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