Co-existence and switching between fast and Ω-slow wind solutions in rapidly rotating massive stars
Sign Up to like & getrecommendations! Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
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