Toward a better understanding of the mid-infrared emission in the Large Magellanic Cloud

Open Access

Fig. 6

Ratio of the PAHs to the large-grain component abundance for the different models and for the ten regions using different RFs (Mathis in black, 4 Myr in red, 60 Myr in blue, and 600 Myr in green). The Galactic value is indicated with the gray line.

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