We discover an average mass-to-light ratio of 1.98 0.03, which is highly consistent with the M/L ratio anticipated if the starting mass function had been a typical Kroupa.
the proportion of an object's mass to its overall brightness. Since solar mass and luminosity are the standard units for measuring mass and brightness, the Sun's mass to light ratio is 1.
The mass-to-light ratio (M/L or ) is the relationship between the stellar mass and brightness of a given population of stars, such as the population in a specific region of space. The value is frequently scaled so that the Sun's M/L is 1, or solar masses to solar luminosities.
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