Fig. 2.
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Integrated emission of H2 S(5) line at 6.91 μm toward GSS30-IRS 1, ISO-Oph 137, [GY92] 197, and WL 17. The positions of the protostars, measured from the line-free region at 6.9 μm, are shown with black stars. The red arrows shows the apparent outflow direction based on the H2 emission. The filled black circle marks the spatial resolution of MIRI at λ = 6.9 μm (∼0.2″).
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