Stellar Winds from Young Stars

Published under licence by IOP Publishing Ltd
, , Citation Nino Panagia 1985 Phys. Scr. 1985 71 DOI 10.1088/0031-8949/1985/T11/010

1402-4896/1985/T11/71

Abstract

The statistical properties of winds from young (pre-main-sequence: PMS) stars are summarized and discussed. One and the same mechanism, possibly related to the process of star formation, appears to be responsible for mass loss in all PMS stars. Moreover, evidence is found that the ionization and the acceleration of the winds of very young stars are produced by processes different from those operating in main sequence and more evolved stars.

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10.1088/0031-8949/1985/T11/010