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Wind Properties of Young Stars

Published online by Cambridge University Press:  04 August 2017

Nino Panagia
Nino Panagia*
Affiliation:
Space Telescope Science Institute, Baltimore, USA

Extract

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The statistical properties of winds form young 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 pre-main-sequence 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.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 398
Copyright
Copyright © Reidel 1987