معرفی
Costanza Argiroffi is a researcher at the University of Palermo within the Department of Physics and Chemistry - Emilio Segrè. Her office hours are scheduled for multiple programs including Physics, Natural and Environmental Sciences, and Optics and Optometry.
- Stellar Evolution (Physics)
- Instrumentation for Optics and Astronomy (Optics and Optometry)
- Accretion processes in young stars
Her research focuses on high-energy astrophysical phenomena, particularly X-ray and UV emission from young stellar objects, magnetohydrodynamic modeling of accretion shocks, and multi-wavelength diagnostics of stellar activity. Publications span topics from stellar flares to laboratory astrophysics and accretion dynamics.
Costanza Argiroffi's recent publications demonstrate strong expertise in:
- X-ray astronomy (XMM-Newton, Chandra, NuSTAR)
- Magnetohydrodynamic simulations
- Young stellar object variability
- Accretion processes in classical T Tauri stars
- Binary star magnetospheres
- Planetary atmosphere irradiation
She has advised multiple theses and participated in research projects involving international collaborations with X-ray observatories.
