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Unveiling stellar aurorae: Simulating auroral emission lines in hot stars induced by high-energy irradiation

By Michal Kajan and others
Auroral emission lines result from the interaction between magnetic field and stellar wind, offering valuable insights into physical properties and processes occurring within magnetospheres of celestial bodies. While extensively studied in planetary and exoplanetary atmospheres, in ultra-cool dwarfs, and as radio emission from early-type stars, the presence of specific auroral... Show more
May 16, 2024
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Unveiling stellar aurorae: Simulating auroral emission lines in hot stars induced by high-energy irradiation
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