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The HCN-water ratio in the planet formation region of disks

Astrophysical Journal (2013) 766(2)
DOI: 10.1088/0004-637X/766/2/134
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Abstract

We find a trend between the mid-infrared HCN/H2O flux ratio and submillimeter disk mass among T Tauri stars in Taurus. While it may seem puzzling that the molecular emission properties of the inner disk (

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Najita, J. R., Carr, J. S., Pontoppidan, K. M., Salyk, C., Van Dishoeck, E. F., & Blake, G. A. (2013). The HCN-water ratio in the planet formation region of disks. Astrophysical Journal, 766(2). https://doi.org/10.1088/0004-637X/766/2/134

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