CI observations in the CQ Tau proto-planetary disk: evidence for a very low gas-to-dust ratio ?

Abstract

Gas and dust dissipation processes of proto-planetary disks are hardly known. Transition disks between Class II (proto-planetary disks) and Class III (debris disks) remain difficult to detect. We investigate the carbon chemistry of the peculiar CQ Tau gas disk. It is likely a transition disk because it exhibits weak CO emission with a relatively strong millimeter continuum, indicating that the disk might be currently dissipating its gas content. We used APEX to observe the two CI lines at 492GHz and 809 GHz in the disk orbiting CQ Tau. We compare the observations to several chemical model predictions. We focus our study on the influence of the stellar UV radiation shape and gas-to-dust ratio. We did not detect the CI lines. However, our upper limits are deep enough to exclude high-CI models. The only available models compatible with our limits imply very low gas-to-dust ratio, of the order of a few, only. These observations strengthen the hypothesis that CQ Tau is likely a transition disk and suggest that gas disappears before dust.

5 pages, 5 figures, accepted for publication in A&A

References in corpus (7)

• Low sulfur depletion in the Horsehead PDR
• Line Emission from Gas in Optically Thick Dust Disks around Young Stars
• Disks around CQ Tau and MWC 758: dense PDR or gas dispersal?
• Chemistry and line emission from evolving Herbig Ae disks
• Atomic Diagnostics of X-ray Irradiated Protoplanetary Disks
• Warm molecular gas and kinematics in the disc around HD 100546
• Molecular line radiative transfer in protoplanetary disks: Monte Carlo simulations versus approximate methods

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• Uncertainties in water chemistry in disks: An application to TW Hya
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