We present upgraded Giant Metrewave Radio Telescope (uGMRT) observations of 0731+438, an radio galaxy at a redshift of 2. 429 with two lobes separated by 82 kpc. A blueshifted, faint, and broad 21 cm absorption line with a velocity full width at half maximum of ∼ 600, ̊m FR II H i -1 is detected against the southern radio lobe that is 47 kpc from radio core, indicating a neutral hydrogen outflow associated with jet-gas interaction beyond the host galaxy. The outflow has a mass outflow rate of ∼, 0. 4T_ ̊m s M_⊙, ̊m yr ^ -1, which could increase to ∼, 4. 0T_ ̊m s ̊m yr ^ -1, corresponding to an energy outflow rate of 2. 4T_ ̊m s Ω -- 1. 5T_ 40 ̊m s Ω, ̊m erg, s^, where T_̊m s is the spin temperature and Ω is the solid angle of the outflow. Previous optical observations identified an extended emission line region aligned with the radio axis, ionized by the central active galactic nucleus (AGN). Within this region, a warm and ionized outflow with a mass outflow rate of ∼, 50̊m, M_⊙, 41 -1 ̊m yr ^ -1 and an energy outflow rate of sim1. 7, ̊m erg, s^ was detected. We propose that both the extended emission line region and the optical outflow are results of a synergistic effect between the jet and AGN radiation. The AGN likely exerts negative feedback on the host galaxy, as is evidenced by the gas expulsion by the jet and the high-velocity dispersion of ionized gas observed optically. So far, detections of jet-driven neutral hydrogen outflows remain rare. The high redshift, large outflow radii, substantial mass outflow rate, and energy outflow rate of the neutral hydrogen outflow in 0731+438 expand the known parameter space of such outflows. Finally, we find tentative correlations between the neutral hydrogen mass outflow rate (or energy outflow rate) and the rest-frame radio power of jets for the known broad neutral hydrogen outflows. 43 -1 1. 4 GHz
Su et al. (Fri,) studied this question.