Effective temperature
= Effective temperature
{title2=$T_{\rm eff}$}
{wiki}
The effective temperature is the temperature of a blackbody with the same radiative flux as a star: $L=4\pi R^2\sigma T_{\rm eff}^4$.
= Effective temperature
{title2=$T_{\rm eff}$}
{wiki}
The effective temperature is the temperature of a blackbody with the same radiative flux as a star: $L=4\pi R^2\sigma T_{\rm eff}^4$.