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Lifetimes of stars in the main sequence and the maximum mass of stars in the galactic disk
Authors:V A Zakhozhay
Institution:1. Karazin National University, pl. Svobody 4, Kharkiv, 61077, Ukraine
Abstract:Generalized and interconsistent approximation formulas are derived to describe the relationship between the hydrogen-burning time and the zero-age stellar mass for the mass and elemental composition ranges characteristic of stars that have been formed during the lifetime of the universe. The maximum masses of population I stars are estimated based on the known statistical relationships among stellar characteristics that agree with observational data.
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