Co-existence and switching between fast and Ω-slow wind solutions in rapidly rotating massive stars
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DOI: 10.1093/mnras/sty678
Abstract: Most radiatively-driven massive star winds can be modelled with m-CAK theory resulting in so called fast solution. However, those most rapidly rotating among them, especially when the stellar rotational speed is higher than $\sim 75\%$… read more here.
Keywords: existence; region; solution; omega slow ... See more keywords
Absence of the strahl during times of slow wind
Sign Up to like & getrecommendations! Published in 2017 at "Annales Geophysicae"
DOI: 10.5194/angeo-35-71-2017
Abstract: Abstract. It is not uncommon during periods when the solar wind speed is less than 425 km s −1 to observe near 1 AU no evidence of a strahl population in either the electron solar… read more here.
Keywords: wind; absence strahl; times slow; slow wind ... See more keywords