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Meredith L. Rawls edited figures/agevsmass_draft/caption.tex
over 8 years ago
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\label{fig:mesa} Ages for a suite of stellar evolution models for stars
ranging from 2.04 to 2.26 $M_{\odot}$ in increments of
0.02. 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
blue lines corresponding to the radii both stars
(solid, (solid black, $R_1 = 7.90 \ R_\odot$;
dashed, dashed blue, $R_2 = 8.33 \ R_\odot$) are shown, along with two vertical lines corresponding to $M_1 = 2.16 \ M_\odot$ and $M_2 = 2.14 \ M_\odot$. This indicates that the two stars in KIC 9246715 are both on the RGB and have a coeval history.
\textbf{NEW AND UPDATED FIGURE COMING SOON!}