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The relationship between mass and luminosity for main sequence stars is such that O luminosity is independent of the stellar mass. O The greater the
The relationship between mass and luminosity for main sequence stars is such that O luminosity is independent of the stellar mass. O The greater the stellar mass, the lower the luminosity The greater the stellar mass, the higher the luminosity. O the luminosity of stars reaches a peak at around 1 solar mass, and decreases as mass increases and decreases beyond this limit
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