2026/03/20 by Hannah Übler, Roberto Maiolino, Pablo G. Pérez-González +32 · 1 voice
#astro-ph.GA #astro-ph.CO
According to the leading cosmological model, a first generation of stars called Population III (PopIII), condensed almost entirely out of hydrogen and helium, must have initiated the creation of all heavier chemical elements. We report the detection of ionised hydrogen (Hγ4342) with a signal-to-noise ratio of S/N=5.9 in a region about 3 pkpc (projected) north-east from the z~10.6 galaxy GN-z11, where line emission compatible with doubly ionised helium (HeII1640) has been found. Our new JWST/NIRSpec-IFU G395H data confirm the authenticity of the previous detection at a redshift of z\rm Hγ=10.5862±0.0003. Hδ is marginally detected (S/N∼2). No metal lines are detected in our observations spanning λ\rm rest=0.25-0.45μm. We derive a 3σ upper limit on the gas phase metallicity of 12+log(O/H)<7.0 (Z\rm gas<0.02 Z_\odot). Through comparison with NIRCam imaging, we constrain a lower limit on the equivalent width of EW0(Hγ)>350Å. We compare our emission line constraints to model predictions and find them compatible with photoionisation by PopIII stars, possibly intermixed with next-generation (PopII) stars. We infer an upper limit on the dynamical mass of M\rm dyn\lesssim3×108M_\odot. Our data provide novel support for the presence of PopIII stars nearby GN-z11, 440 Myr after the Big Bang.