Surface gravity along the main sequence.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Main-Sequence Stars: Surface Gravity

Scientific paper

On the basis of the empirical distributions of the radii and critical rotation velocities for normal stars an analysis concerning the surface-gravity (g(M)) distribution along the main sequence is undertaken. It appears that g(M) is largely determined by the R-1(M) distribution, especially in the region of rapid changes (about M = 1.2 - 1.4 Msun).

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