Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.
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Gas chemistry in the dust depleted inner regions of protoplanetary disks. I. Near-IR spectra and overtones
Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.