Now showing items 1-1 of 1

    • A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk. 

      Berné, O; Habart, E; Peeters, E; Schroetter, I; Canin, A; Sidhu, A; Chown, R; Bron, E; Haworth, TJ; Klaassen, P (2024-03)
      Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photodissociation regions ...