Role of local absorption on the X-ray emission from MHD accretion shocks in classical T Tauri stars
Accretion processes onto classical T Tauri stars (CTTSs) are believed to generate shocks at the stellar surface due to the impact of supersonic downflowing plasma.Although current models of accretion streams provide a plausible global picture of Ball - Bat - Fungo this process, several aspects are still unclear.For example, the observed X-ray lumin