(b) Strong mass loss will occur at the surface of stars when the radiation pressure gradient exceeds that required by hy
Posted: Mon May 23, 2022 10:15 am
(b) Strong mass loss will occur at the surface of stars when the radiation pressure gradient exceeds that required by hydrostatic equilibrium. Show that the maximum mass of a star with a surface stable to radiation pressure driven mass loss is: OTL Mmax = 49Gcmp 7 where L is the luminosity of the star. Assume that electron scattering is the dominant source of opacity and that à ~ otp/mp, where or is the cross section for electron scattering and p is the gas density. р