MINDS: The DR Tau disk - I. Combining JWST-MIRI data with high-resolution CO spectra to characterise the hot gas

Open Access

Fig. 5

Zoom-in on the ¹²CO₂ Q branch (14.80–15.05 µm) of GW Lup (left; Grant et al. 2023) and DR Tau (right). Both spectra have been scaled to a common distance of 150 pc and normalised to the peak of the ¹²CO₂ Q branch.

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