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 this process, several aspects are still unclear. For...
Main Authors: | Bonito, Orlando, Argiroffi, Miceli, Reale, Peres, Matsakos, Stehle, Ibgui |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2014-01-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20136405004 |
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