Interpreting ALMA non-detections of JWST super-early galaxies
arXiv:2212.02519 · doi:10.1093/mnrasl/slac166
Abstract
Recent attempts to detect [OIII] 88m emission from super-early () galaxy candidates observed by JWST have been unsuccessful. By using zoom-in simulations, we show that these galaxies are faint, and mostly fall below the local metal-poor relation as a result of their low ionization parameter, . Such low values are found in galaxies that are in an early assembly stage, and whose stars are still embedded in high-density natal clouds. However, the most luminous galaxy in our sample (, ) could be detected by ALMA in only hrs.
6 pages, 3 figures, Submitted to MNRAS (comments are welcome)
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