deletions | additions       diff --git a/figures/sketch/caption.tex b/figures/sketch/caption.tex  index 22ec9e8..3c454c1 100644  --- a/figures/sketch/caption.tex  +++ b/figures/sketch/caption.tex 
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\label{fig:sketch}  Geometry in the $(r,z)$ $(z,\bar{\omega})$  plane. The $z$-axis is oriented along the jet, the $r$-axis $\bar{\omega}$-axis  in the plane of the circumstellar accretion disk. The innermost outflow layer is the unshocked stellar wind. The shock front is located at $R_{\rm{shock}}(z)$. The next layer is hot, post-shock stellar wind, which is separated from the disk wind by the contact discontinuity at $R_{\rm{contdisc}}(z)$.