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Modules for Experiments in Stellar Astrophysics (MESA)

  • Authors: Bill Paxton, Lars Bildsten, Aaron Dotter, Falk Herwig, Pierre Lesaffre, and Frank Timmes

Paxton et al. 2011 The Astrophysical Journal Supplement Series 192 3.

  • Provider: AAS Journals

Caption: Figure 15.

Location in the Hertzsprung-Russell (H-R) diagram for 0.085  M < M < 1  M stars as they arrive at the main sequence for Y = 0.275 and Z = 0.019. The mass of the star is noted by the values at the bottom of the line. The dashed blue lines are isochrones for ages of 3, 10, 30, 100 and 300 Myr, as noted to the right. The purple squares (red circles) show where D ( 7Li) is depleted by a factor of 100. The green triangles show the ZAMS.

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