Stellar evolution

  • Article
    | Open Access

    The ionisation fraction of protostellar jets is key to establish their true energetics. Here, the authors determine it in a jet from a high-mass young stellar object, using multi-wavelengths observations, confirming that the ionising mechanism giving rise to the radio emission originates from shocks.

    • R. Fedriani
    • , A. Caratti o Garatti
    •  & M. Hoare