A massive galaxy at z=9.3 shows bursty star formation with a recent downturn and sits in a small ionized bubble in a neutral IGM.
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Rest-frame UV spectra of two z~8.7 galaxies reveal strong P-Cygni wind profiles and HeII emission best reproduced by stellar population models that include very massive stars, implying an IMF extending beyond 100 solar masses.
citing papers explorer
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SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$
A massive galaxy at z=9.3 shows bursty star formation with a recent downturn and sits in a small ionized bubble in a neutral IGM.
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Signatures of Very Massive Stars in the Epoch of Reionization
Rest-frame UV spectra of two z~8.7 galaxies reveal strong P-Cygni wind profiles and HeII emission best reproduced by stellar population models that include very massive stars, implying an IMF extending beyond 100 solar masses.