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Neon Fine-Structure Line Emission By X-ray Irradiated Protoplanetary Disks
ASTROPHYSICAL JOURNAL, no. 1 (2007): 515-523
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Using a thermal-chemical model for the generic T Tauri disk of D'Alessio and colleagues, we estimate the strength of the fine-structure emission lines of Ne II and Ne III at 12.81 and 15.55 mu m that arise from the warm atmosphere of the disk exposed to hard stellar X-rays. The Ne ions are produced by the absorption of keV X-rays from the...More
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