Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.
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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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Disc lifetime distribution as a function of the mass of host star
Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.
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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.