Pamela Freeman edited figures/massradius/caption.tex  about 8 years ago

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The luminous mass $M_{lum}$ $M_\mathrm{lum}$  as a function of the radius $R$ for GMCs, colored by galactocentric distance $R_{gal}$. $R_\mathrm{gal}$.  Fit lines are for M83 (blue line) and the Milky Way (green line, from Solomon et al. 1987). \label{fig:rm}