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Optical and X-ray variability in pre Main Sequence Stars of NGC 2264 | Mario Guarcello ( INAF-Osservatorio Astronomico di Palermo)
@ Aula OAPA
Optical and X-ray variability in pre Main Sequence Stars of NGC 2264 | Mario Guarcello ( INAF-Osservatorio Astronomico di Palermo)
@ Aula OAPA
Nov 27 @ 15:30 – 16:30
Young stars are known to be variable sources both in optical, infrared, and X-ray. This variability is strictly correlated with their physical properties and the morphology of the circumstellar material, if any. The study of their light curves and the connection between the observed variability in the various regions of the electromagnetic spectrum provides a deep insight on the physical
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