Meredith L. Rawls edited figures/agevsmass_draft/caption.tex  almost 9 years ago

Commit id: 12b04df6511bee9edb0c2a073da516bc3763c675

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\label{fig:mesa} Ages for a suite of simple stellar evolution models for stars ranging from 2.04 to 2.26 $M_{\odot}$ in increments of 0.02. Color indicates the evolutionary state of each star as it moves from the Main Sequence (MS) $\rightarrow$ Red Giant Branch (RGB) $\rightarrow$ Secondary Red Clump/Horizontal Branch (HB) $\rightarrow$ Asymptotic Giant Branch and beyond (AGB+). Two blue lines corresponding to the radii of Star 1 (solid, $R = 7.90 \ R_\odot$) and Star 2 (dashed, $R = 8.33 \ R_\odot$) are shown. This suggests that the two stars in KIC 9246715 (with masses $2.16$ and $2.14 \ M_\odot$, respectively) are both on the RGB and have a coeval history.  \textbf{JEAN: PLEASE PROVIDE AN UPDATED VERSION OF THIS FIGURE WITH A SUITE OF MASS-VARYING MODELS GENERATED THE SAME WAY AS YOUR 'LOGS_9246715_star2_ov_2' `LOGS_9246715_star2_ov_2'  MESA RUN. THE AGES WILL BE SLIGHTLY DIFFERENT.}