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The Large‐Scale J = 3 → 2 and J = 2 → 1 CO Emission from M17 and Its Implications for Extragalactic CO Observations

  • Authors: Christine D. Wilson, John E. Howe, and Michael L. Balogh

Wilson, Howe, & Balogh 1999 The Astrophysical Journal 517 174.

  • Provider: AAS Journals

Caption: Fig. 6.

LVG solution at a kinetic temperature ﹩T_{K}=30﹩ K for the CO line ratios for M17 averaged over the entire cloud. The lines indicate the observed ±1 σ values for the line ratios 12CO/13CO ﹩J=2\rightarrow 1﹩ (﹩4.5\pm 0.7﹩; solid line); 12CO/13CO ﹩J=3\rightarrow 2﹩ (﹩3.7\pm 0.9﹩; dashed line); 12CO (﹩J=3\rightarrow 2﹩)/(﹩J=2\rightarrow 1﹩) (﹩0.76\pm 0.19﹩; dot‐dashed line; lower limit in lower left corner, upper limit along lower right); and 13CO (﹩J=3\rightarrow 2﹩)/(﹩J=2\rightarrow 1﹩) (﹩1.3\pm 0.3﹩; dotted line; only the lower limit appears in the figure). The hatched area indicates the region where all four sets of lines intersect, and the black area encompasses the region where ﹩\Delta \chi ^{2}\leq 1﹩.

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