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15:30
Role of local absorption on the X-ray emission from MHD accretion shocks in classical T Tauri stars | Sara Bonito (INAF – Osservatorio Astronomico di Palermo)
@ Aula OAPA
Role of local absorption on the X-ray emission from MHD accretion shocks in classical T Tauri stars | Sara Bonito (INAF – Osservatorio Astronomico di Palermo)
@ Aula OAPA
Jul 23 @ 15:30 – 16:30
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 this process, several aspects are still unclear. For example, the observed X-ray luminosity in accretion shocks is, in general, well below the predicted
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