No CrossRef data available.
Article contents
Turbulence in Main Sequence Stars
Published online by Cambridge University Press: 12 April 2016
Extract
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
- Copyright
- Copyright © Springer-Verlag 1980