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Water Formation During the Epoch of First Metal Enrichment
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abstract
We demonstrate that high abundances of water vapor could have existed in extremely low metallicity ($10^{-3}$ solar) partially shielded gas, during the epoch of first metal enrichment of the interstellar medium of galaxies at high redshifts.
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Cited by 1 Pith paper
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Abundant Water from Early Supernovae at Cosmic Dawn
Cosmological simulations find that dense cores in the remnants of the first supernovae synthesized water with mass fractions up to 10^-4 by redshift z~20.
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