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. 4.

Fe feature in the spectrum of the hot spot (see Fig. 3). Only some relevant simulations are shown. (ρ = 10¹⁶ cm s⁻³, K = 800 keV) is marked in black, (ρ = 10¹⁷ cm s⁻³, K = 800 keV) is marked in purple, (ρ = 10¹⁶ cm s⁻³, K = 1, 600 keV) is marked in green, and (ρ = 10¹⁷ cm s⁻³, K = 1600 keV) is marked in brown.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.