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    • Upper limits to ultraviolet line emission in fully convective M-dwarfs 

      Ambruster, C. W.; Kunkel, W. E.; Moreno, H.; Basri, G. B. (1986)
      Theoretical stellar structure models find that stars later than ∼dM3 are fully convective. It is widely believed that this should result in reduced non-radiative heating and activity levels, however, the observational ...