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    • The ramp-up of interstellar medium enrichment at z>4 

      Franco, M.; Coppin, K. E. K.; Geach, J. E.; Kobayashi, C.; Chapman, S. C.; Yang, C.; González-Alfonso, E.; Spilker, J. S.; Cooray, A.; Michałowski, M. J. (2021-11-04)
      Fluorine is one of the most interesting elements for nuclear and stellar astrophysics 1,2. Fluorine abundance was first measured for stars other than the Sun in 1992 1, then for a handful of metal-poor stars 3, which are ...