For stars of the solar type, the following dependence of the luminosity L on the mass M is characteristic: L ~ M ^ 4 Main

For stars of the solar type, the following dependence of the luminosity L on the mass M is characteristic: L ~ M ^ 4 Main sequence stars with what masses can be in the vicinity of the Sun, if we assume that they were formed simultaneously with the Sun? Why?

With masses of up to 1.3 solar masses (stars of large masses have left the main sequence during the lifetime of the Sun).

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