Observational Consequences of Turbulent Pressure in the Envelopes of Massive Stars
The major mass fraction of the envelope of hot luminous stars is radiatively stable. However, the partial ionization of hydrogen, helium, and iron gives rise to extended sub-surface convection zones in all of them. In this work, we investigate the effect of the pressure induced by the turbulent motion in these zones based on the mixing-length
Grassitelli, L. et al.
Fecha de publicación:
7
2015