Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4

Abstract

We report the discovery and analysis of only the third Lyman-limit system in which a high-quality resolution, echelle spectrum reveals no metal absorption lines, implying a metallicity $\lesssim$1/10000 solar. Our HIRES spectrum of the background quasar, PSS1723$+$2243, provides a neutral hydrogen column density range for LLS1723 of $N_{\text{HI}}=10^{\text{17.9–18.3}}$ cm${}^{-2}$ at redshift $z_{\text{abs}}\approx 4.391$. The lower bound on this range, and the lack of detectable absorption from the strongest low-ionisation metal lines, are combined in photoionisation models to infer a robust, conservative upper limit on the metallicity: $\log (Z/Z_{\odot })<-4.14$ at 95% confidence. Such a low metallicity raises the question of LLS1723's origin and enrichment history. Previous simulations of the circumgalactic medium imply that LLS1723 is a natural candidate for a cold gas stream accreting towards a galaxy. Alternatively, LLS1723 may represent a high-density portion of the intergalactic medium containing either pristine gas -- unpolluted by stellar debris for 1.4 Gyr after the Big Bang -- or the remnants of low-energy supernovae from (likely low-mass) Population III stars. Evidence for the circumgalactic scenario could be obtained by mapping the environment around LLS1723 with optical integral-field spectroscopy. The intergalactic possibilities highlight the need for -- and opportunity to test -- simulations of the frequency with which such high-density, very low-metallicity systems arise in the intergalactic medium.

arXiv comment12 pages, 6 figures, 1 table, accepted for publication in MNRAS

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