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Redshift in the X-ray emission of TW~Hya: indication of a low-latitude accretion spot | Costanza Argiroffi (Dip. di Fisica e Chimica, Universita’ di Palermo)
@ Aula OAPa
Redshift in the X-ray emission of TW~Hya: indication of a low-latitude accretion spot | Costanza Argiroffi (Dip. di Fisica e Chimica, Universita’ di Palermo)
@ Aula OAPa
Dec 5 @ 15:30
High resolution spectroscopy, providing constraints on plasma motions and temperatures, is a powerful means to investigate the structure of accretion streams in Classical T Tauri stars (CTTS). In particular the accretion-shock region, where the accreting material is heated to temperatures of a few million degrees, can be probed by X-ray spectroscopy. MHD models predict that this hot post-shock plasma should
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