deletions | additions       diff --git a/figures/kernel_omega/caption.tex b/figures/kernel_omega/caption.tex  index 39bc7d8..c748849 100644  --- a/figures/kernel_omega/caption.tex  +++ b/figures/kernel_omega/caption.tex 
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ADIPLS calculations of the integrated kernels for g-dominated (yellow and red) and p-dominated (blue) mixed modes in one of our models. The x-axis is showing the normalized radial coordinate. Solid lines are for $\ell=1$ and dashed lines for $\ell=2$. The black solid line represents the angular velocity profile of the background structure model calculated with MESA. The convective envelope is shown in grey, while the location of the H-burning shell is marked in turquoise. The background model has an initial mass of $1.5\mso$, an initial equatorial rotational velocity of $50\kms$ and has been evolved including the effect of magnetic torques from Tayler-Spruit dynamo fields \label{kernels}. fields\label{kernels}.