Fig. 4 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. 4.

Radius vs. time diagram for stellar models with mass ranging from 0.08 M_☉ to 0.25 M_☉. In each sequence of models (except for the 0.25 M_☉ model) a maximum radius is reached, and at the very latest times plotted, the radius is shrinking.

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