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Adiabatic Mass Loss in Binary Stars. III. From the Base of the Red Giant Branch to the Tip of the Asymptotic Giant Branch

  • Authors: Hongwei Ge, Ronald F Webbink, Xuefei Chen, and Zhanwen Han

2020 The Astrophysical Journal 899 132.

  • Provider: AAS Journals

Caption: Figure 1.

Evolutionary track of a ﹩3.2\,{M}_{\odot }﹩ star in the Hertzsprung–Russell diagram. The models we choose to study in its evolutionary track are labeled with solid dots and circles. The thin dotted line of the evolutionary track signifies evolutionary phases in which the stellar radius is smaller than in the preceding phase. Seven major evolutionary phases are labeled.

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