TL;DR
This paper reports the discovery of a high-redshift molecular outflow in a hyperstarburst galaxy, revealing a transient, intense star formation phase with outflows unable to regulate star formation, suggesting rapid gas consumption.
Contribution
First detection of a high-redshift molecular outflow in a hyperstarburst galaxy using water absorption lines with ALMA, providing insights into extreme star formation and feedback processes.
Findings
Outflow rate of ~500 M_sun/year, lower than SFR, indicating saturated outflow capability.
Star formation rate surface density exceeds Eddington limit, implying a transient starburst phase.
Galaxy is a single starburst with a surrounding disc, not a merger.
Abstract
We report the discovery of a high-redshift, massive molecular outflow in the starburst galaxy SPT0346-52 () via the detected absorption of high-excitation water transitions (HO and HO ) with the Atacama Large Millimeter/submillimeter Array (ALMA). The host galaxy is one of the most powerful starburst galaxies at high redshift (star formation rate; SFR Myear), with an extremely compact (pc) star formation region and a star formation rate surface density (Myearkpc) five times higher than `maximum' (i.e. Eddington-limited) starbursts, implying a highly transient phase. The estimated outflow rate is Myear, which is much lower than the SFR, implying that in this extreme starburst the outflow capabilities saturate and the outflow is…
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