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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. 5.

Radius vs. luminosity as a function of helium enrichment for the alternate sequence of stellar models with mass M* = 0.20 M☉. The models with depleted hydrogen (helium enrichment) start their evolution at considerably larger luminosities and show much smaller increases in radii.

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