Erik Rosolowsky edited figures/Rlinewidth_matplotlib (1)/caption.tex  about 8 years ago

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Figure 2. The velocity line width $\sigma$ against the radius $R$ for the clouds, color coded by galactocentric distance $R_{gal}$. Fit lines are for M83 (blue line) and the Milky Way (green line, from Solomon et al. 1987). \label{fig:rdv}