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    • Non-thermal radio continuum emission from young nearby stars 

      Launhardt, R.; Loinard, Laurent; Dzib, Sergio A.; Forbrich, J.; Bower, G. C.; Henning, Th K.; Mioduszewski, A. J.; Reffert, S. (2022-05-23)
      Young and magnetically active low-mass stars often exhibit non-thermal coronal radio emission due to the gyration of electrons in their magnetized chromospheres. This emission is easily detectable at centimeter wavelengths ...