The β Pictoris system: Setting constraints on the planet and the disk structures at mid-IR wavelengths with NEAR

Open Access

Fig. 14

Projected distribution of CO lines flux obtained from Dent et al. (2014) and Matrà et al. (2017), superimposed with the radial flux distribution of the disk at 12µm with VISIR. The VISIR and CO 3–2 (Dent et al. 2014) curves have beennormalized bytheirmaximum.

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