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MESA ISOCHRONES AND STELLAR TRACKS (MIST) 0: METHODS FOR THE CONSTRUCTION OF STELLAR ISOCHRONES

  • Authors: Aaron Dotter

2016 The Astrophysical Journal Supplement Series 222 8.

  • Provider: AAS Journals

Caption: Figure 8.

This figure shows how the primary and secondary EEPs are distributed along three stellar evolution tracks with Minit = 0.95, 1, and 1.05 M. The original tracks are plotted as solid lines; the secondary EEPs are shown as small dots and the primary EEPs are shown as large dots. This should give some indication that the EEP-based tracks constitute a uniform basis.

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