Abstract:Resumen en: All main sequence stars lose mass via stellar winds. The winds of cool stars like the sun are driven by gas pressure gradient. However, the winds of hot ......Resumen en: All main sequence stars lose mass via stellar winds. The winds of cool stars like the sun are driven by gas pressure gradient. However, the winds of hot ...Read More
Publication Year: 2010
Publication Date: 2010-12-01
Language: en
Type: article
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