Fig. 2 from The End of the Main Sequence

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The End of the Main Sequence

Authors: Gregory Laughlin, Peter Bodenheimer, and Fred C. Adams

Laughlin, Bodenheimer, & Adams 1997 The Astrophysical Journal 482 420.

Provider: AAS Journals

Caption: Fig. 2.

Evolution in the Hertzsprung‐Russell diagram for stars with masses in the range 0.06 M_☉ ≤ M_* ≤ 0.25 M_☉. The inset diagram shows the corresponding main‐sequence lifetimes as a function of stellar mass.

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