deletions | additions       diff --git a/figures/p_rot_jconv/caption.tex b/figures/p_rot_jconv/caption.tex  index 2519e5e..e76e4fe 100644  --- a/figures/p_rot_jconv/caption.tex  +++ b/figures/p_rot_jconv/caption.tex 
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Like Fig.~\ref{period_evolution} but showing only the evolution past He ignition. Different lines show the core rotation rate for 1.5, 2.0 and 3.0 $\mso$ models initially rotating with 50, 50 and 150 $\kms$ respectively. All models include Tayler-Spruit magnetic fields. The black line shows the surface rotational period of the 1.5$\mso$ model. Final rotational period for the 1.5,2.0 and 3.0$\mso$ of \citet{larends_Yoon_Heger_Herwig_2008} are shown by star symbols. These models have also been calculated including magnetic torques but with initial rotational velocities 45, 140 and 250 $\kms$ respectively. The 1.5$\mso$ model ignites He in a degenerate core, resulting in a $\sim 2 $ Myr phase in which the degeneracy is removed through repeated convective events (He-core flash). \label{pzoom}