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The Impact of Pollution on Stellar Evolution Models

  • Authors: Aaron Dotter and Brian Chaboyer

Dotter & Chaboyer 2003 The Astrophysical Journal 596 496.

  • Provider: AAS Journals

Caption: Fig. 3.

Top panel: Comparison of the dispersion in the Hyades sample (thick line) and the average of the mock data sets with mean pollution of 1.0 M (thin line); 90% confidence bands are drawn for the dispersion in the data (dotted lines) and the mock data sets (dashed lines). Bottom panel: Same as the top panel but for the 0.5 M case.

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