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Correlated optical and X-ray variability in Classical T Tauri Stars | E. Flaccomio ( INAF- Osservatorio Astronomico di Palermo )
@ Aula OAPA
Correlated optical and X-ray variability in Classical T Tauri Stars | E. Flaccomio ( INAF- Osservatorio Astronomico di Palermo )
@ Aula OAPA
Mar 3 @ 15:30 – 16:30
Young stars in the Classical T Tauri phase are characterized by complex and highly dynamical phenomena involving the stars, their circumstellar disks, mass accretion, and outflows. Quite unsurprisingly, high energy processes, as traced by, e.g., the X-ray emission, are affected or even driven by the interaction between these components. Because of the widely different characteristic temperatures of the involved physical
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