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CHEMICAL COMPOSITION OF INTERMEDIATE-MASS STAR MEMBERS OF THE M6 (NGC 6405) OPEN CLUSTER

  • Authors: T. Kılıçoğlu, R. Monier, J. Richer, L. Fossati, and B. Albayrak

2016 The Astronomical Journal 151 49.

  • Provider: AAS Journals

Caption: Figure 13.

Radiative acceleration profiles from XEVOL for a number of elements in the 4.7 ﹩\;{M}_{\odot }﹩ model T150KD1K-3. Profiles are shown for ages 2 Myr (green), 50 Myr (gray), and 85 Myr (red). The horizontal dotted curves show the run of log g through the envelope, while vertical lines show the limits of envelope convection zones for He II (dotted) and iron group elements (solid, if present).

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