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2016 Aug September 2017 Oct 2018
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VideoConf scuola INAF-SAIt Padova 10:45
VideoConf scuola INAF-SAIt Padova @ Aula virtuale GARR/VCONF
Sep 1 @ 10:45 – 13:15
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SEMINARIO: Constraining the structure of the accretion-shock region in CTTS: possible XMM+HST observing program / Costanza Argiroffi (UNIPA/OAPA) 15:00
SEMINARIO: Constraining the structure of the accretion-shock region in CTTS: possible XMM+HST observing program / Costanza Argiroffi (UNIPA/OAPA)
Sep 18 @ 15:00 – 16:00
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Classical T Tauri stars are bright in the soft X-ray and far UV bands, because of large amounts of plasma at T~105-106 K, associated with the accretion-shock regions. Inspecting the emission from the shock region is important since it can potentially reveal fundamental properties of the accretion-stream material (i.e. geometry/density/velocity/abundances). However, the precise location of these hot plasmas (pre-shock? post-shock?
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2016 Aug September 2017 Oct 2018