In M17, the gas-to-dust ratio inferred from CO and infrared extinction rises from about 118 at low extinction to roughly 300 to 390 at high extinction.
IAU Symposium, https://ui.adsabs.harvard.edu/abs/1997IAUS..170...47A 170
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The Gas-to-Dust Ratio Investigation in the Massive Star-Forming region M17
In M17, the gas-to-dust ratio inferred from CO and infrared extinction rises from about 118 at low extinction to roughly 300 to 390 at high extinction.