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The stochastical approach to the modelling of the line profiles in T Tauri stellar winds

Published online by Cambridge University Press:  23 September 2016

V.P. Grinin  and
A.S. Mitskevich
V.P. Grinin
Affiliation:
Crimean Astrophysical Observatory. P.O. Nauchny, Crimea, 334413 U.S.S.R.
A.S. Mitskevich
Affiliation:
Crimean Astrophysical Observatory. P.O. Nauchny, Crimea, 334413 U.S.S.R.

Abstract

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Line profiles calculations were carried out for spherically-symmetrical stellar wind models with discrete structure. It is shown the possibility to explain two-component emission profiles typical for T Tauri-type stars in the framework of such stochastical approach.

Type
IV Theoretical Problems and Interpretation of Observations
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 343 - 346
Copyright
Copyright © Kluwer 1990