Physics — Stellar Luminosity & Magnitude
Luminosity, the distance modulus and the mass–luminosity relation.
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L = 4\pi R^2 \sigma T^4
m - M = 5\log_{10}\frac{d}{10\,\text{pc}}
\frac{L}{L_\odot} = \left(\frac{M}{M_\odot}\right)^{3.5}
F = \frac{L}{4\pi d^2}