Multi-band observations of stellar flares. the study: “A multi-wavelength view of magnetic flaring from PMS stars” of E. Flaccomio (Inaf – OAPA) recently published by A&A
Most of the stars, mainly the low mass stars, produce their own magnetic field in their interior. The interaction between the magnetic field and stellar plasma is the cause of phenomena such as photosperic spots, faculae, protuberances, coronal mass ejections, and flares. The study of this activity is important both because it reveals how intense magnetic fields interact with high-temperature
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