Mass loss from solar-type stars
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L. Hartmann
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Article
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1985
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Springer
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English
β 656 KB
Winds are directly detected from solar-type stars only when they are very young. At ages ~ 106 yr, these stars have mass loss rates ~ 106 times the mass flux of the present solar wind. Although these young T Tauri stars exhibit ultraviolet transition-region and X-ray coronal emission, the large part