Resurgence of CO in a warm bubble around accreting protoplanets and its observability

Open Access

Fig. 1

Absorption opacities as a function of the wavelength (top) and mean opacities as a function of the temperature (bottom) for populations of small (red; $a_{d}^{small} = 0.1 μ$ $a_{\mathrm{d}}^{\text {small}}=0.1\ \mu$ m) and large (blue; $a_{d}^{large} = 1$ $a_{\mathrm{d}}^{\text {large}}=1$ mm) dust grains. In the bottom panel, the Planck and Rosseland opacities are shown as solid and dashed curves, respectively.

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