MINDS: Mid-infrared atomic and molecular hydrogen lines in the inner disk around a low-mass star

Open Access

Fig. 6

Emission lines used to measure the accretion rates. The black dashed profile on the left is the HI (7-6) line, the one on the right is the HI (11-8) line, while the central component is C₂H₂ emission, according to the predictions of Tabone et al. (2023, the orange profile).

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