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Hans Moritz Günther edited figures/dot_m/caption.tex
almost 10 years ago
Commit id: 5eaf0bfaf41c312254a7c6f4faa8c32a5d9ce105
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\label{fig:dot_m}
Solutions to the ODE for different mass loss rates. For a description of the individual panels see Fig.~\ref{fig:p_ext}. The middle left panel only shows the region close to the star for clarity. The shock front with the largest mass loss rate extends to $\omega=50$~AU
at $z=60$~AU and comes back to the axis of symmetry at 130~AU.