Resolving the HI in Damped Lyman-α systems that power star-formation
arXiv:2205.08554 · doi:10.1038/s41586-022-04616-1
Abstract
Reservoirs of dense atomic gas (primarily hydrogen), contain approximately 90 percent of the neutral gas at a redshift of 3, and contribute to 2-3 percent of the total baryons in the Universe. These damped Lyman- systems (so called because they absorb Lyman- photons from within and from background sources) have been studied for decades, but only through absorption lines present in the spectra of background quasars and gamma-ray bursts. Such pencil beams do not constrain the physical extent of the systems. Here, we report integral-field spectroscopy of a bright, gravitationally lensed galaxy at a redshift of 2.7 with two foreground damped Lyman- systems. These systems are 238 in extent, with column densities of neutral hydrogen varying by more than an order of magnitude on 3 kpc-scales. The mean column densities are - and the total masses are - , showing that they contain the necessary fuel for the next generation of star formation, consistent with relatively massive, low-luminosity primeval galaxies at redshifts 2.
31 pages, 4 Figures, 4 Extended Data figures, 2 Extended Data tables, Author's version, Accepted: 4 March 2022, Published online by Nature on May 18, 2022
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