Source of the Fe Kα emission in T Tauri stars - Radiation induced by relativistic electrons during flares. An application to RY Tau

Open Access

Fig. 3.

Output X-ray spectrum from the hot spot obtained for kinetic energies of the e-beam: 200 keV, 400 keV, 800 keV, and 1.6 MeV (see top), and a media density of 10¹⁴ cm⁻³, 10¹⁵ cm⁻³, 10¹⁶ cm⁻³, and 10¹⁷ cm⁻³. No hot spot is produced for the lowest simulated density N = 10¹³ cm⁻³, nor is there any Fe Kα emission.

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