Issue |
A&A
Volume 564, April 2014
|
|
---|---|---|
Article Number | A57 | |
Number of page(s) | 20 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201323031 | |
Published online | 04 April 2014 |
Online material
Appendix A: Tables of iteration cycles
Iteration cycles for the equatorial wind from a rotating O5–V main-sequence star with Vrot = 300 km s-1 (see upper table) and Vrot = 500 km s-1 (see lower table) without distortion.
Iteration cycles for the wind from an O-giant star rotating with Vrot = 300 km s-1 at the pole (see upper table) and at the equator (see lower table) without distortion.
Iteration cycles for the wind from a rotating O5–V main-sequence star with Vrot = 300 km s-1 at the pole (see upper table) and at the equator (see lower tables) considering the stellar distortion and the effects of gravity darkening.
Iteration cycles for the wind from a rotating O5–V main-sequence star with Vrot = 500 km s-1 at the pole (see upper table) and at the equator (see middle and lower tables) considering the stellar distortion and the effects of gravity darkening.
© ESO, 2014
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