Radiative stellar structure
= Radiative stellar structure
In a radiative stellar region, photons carry luminosity down the temperature gradient. Dimensional scaling of the radiative-diffusion equation gives $L\sim RT_c^4/(\kappa_c\rho_c)$.
= Radiative stellar structure
In a radiative stellar region, photons carry luminosity down the temperature gradient. Dimensional scaling of the radiative-diffusion equation gives $L\sim RT_c^4/(\kappa_c\rho_c)$.