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1 GRAVITY operates in the near-infrared K-band, i.e., with wavelengths between 2 and 2.5 μm. 2 PIONIER at the VLTI operates in the near-infrared H-band, i.e., with wavelengths between 1.5 and 1.8 μm. 3 MATISSE at the VLTI operates in the mid-infrared L-, M-, and N-bands, i.e., with wavelengths between 3 and 13 μm (Lopez et al., 2018). emission we measured with GRAVITY is located at positions smaller than the critical radius where the gap is expected to form as a result of to extreme-/farultraviolet/X-ray heating, the discs in our sample might be shaped by forming young planets rather than by depletion resulting from photoevaporation (Figure 2).

Spatially Resolving the Inner Gaseous Disc of the Herbig Star 51 Oph through its CO Ro-vibration Emission