I was reading Stellar Evolution in Early Phases of Gravitational Contraction, by Chushiro Henyey, where he writes,
If LproptoR−alpha along the path, the age of a star from the time when R=infty is given by
t=C/(1−alpha),C=GM2/RL=107.20left(fracMModotright)2fracRodotRfracLodotLtextyears
where R and L are the present values.
This seems to be just for stars on the Hayashi track (and treated here just for Population 1 stars). Is there a similar expression for stars on the Henyey track, or is the same expression valid in both scenarios?
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