Mass-Luminosity Relation ·
L ∝ M^α
un
seel
.com · Eddington 1924 · α ≈ 4 (solar)
10 M☉ →
10,000 L☉
t
MS
∝
M
−3
phase
—
Massive O/B (short-lived)
Sun-like G
Red dwarf M
L ∝ M⁴ slope
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.com · Mass-Luminosity Relation