a
= a
{scope}
Radiative transport supplies the <temperature> gradient used below. A purely radiative equilibrium model also needs <stellar convective stability>; the transport assumption alone is not a general proof of stability.
= a
{scope}
Radiative transport supplies the <temperature> gradient used below. A purely radiative equilibrium model also needs <stellar convective stability>; the transport assumption alone is not a general proof of stability.