deletions | additions       diff --git a/figures/agevsmass_draft/caption.tex b/figures/agevsmass_draft/caption.tex  index 3de0fe1..ba245bd 100644  --- a/figures/agevsmass_draft/caption.tex  +++ b/figures/agevsmass_draft/caption.tex 
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\label{fig:mesa} Ages for a suite of MESA stellar evolution models for stars of different masses, incremented by $0.01 \ M_\odot$. 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 nearly-overlapping  lines corresponding to the radii radius  of both stars each star are shown  (solid black, $R_1 = 7.90 \ R_\odot$; dashed blue, $R_2 = 8.33 \ R_\odot$) are shown, R_\odot$),  along withtwo  vertical lines corresponding to $M_1 = 2.16 \ M_\odot$ and $M_2 = 2.14 \ M_\odot$. This suggests the stars in KIC 9246715 are both on the RGB, because they would need larger radii to be on the HB. Given the uncertainty in mass (0.03--0.04 $M_\odot$), it is possible for both stars to be the same age on the RGB.