MINDS: The very low-mass star and brown dwarf sample - II. Probing disk settling, dust properties, and dust-gas interplay with JWST/MIRI

Open Access

Fig. 4

Gas column density and spectral slope. $F_{13_{{CCH}_{2}}} / F_{C_{2} H_{2}}$ ${F_{{{13}_{{\rm{CC}}{{\rm{H}}_2}}}}}/{F_{{{\rm{C}}_2}{{\rm{H}}_2}}}$ represents gas column density, measured in Paper I. J1558 is the upper limit value for $F_{13_{{CCH}_{2}}} / F_{C_{2} H_{2}}$ ${F_{{{13}_{{\rm{CC}}{{\rm{H}}_2}}}}}/{F_{{{\rm{C}}_2}{{\rm{H}}_2}}}$ .

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