FAST discovery of a fast neutral hydrogen outflow
Renzhi Su, Minfeng Gu, S. J. Curran, Elizabeth K. Mahony, Ningyu Tang,, James R. Allison, Di Li, Ming Zhu, J. N. H. S. Aditya, Hyein Yoon, Zheng, Zheng, Zhongzu Wu

TL;DR
This paper reports the discovery of a fast neutral hydrogen outflow in a merging radio galaxy using FAST, highlighting the outflow's properties, potential drivers, and implications for AGN feedback.
Contribution
First detection of a fast neutral hydrogen outflow in a merging galaxy with FAST, demonstrating its capability to identify such phenomena and analyzing potential feedback mechanisms.
Findings
Outflow velocity up to -1000 km/s
Mass outflow rate between 0.028 and 3.6 M_sun/yr
Radio jet likely drives the outflow
Abstract
In this letter, we report the discovery of a fast neutral hydrogen outflow in SDSS J145239.38+062738.0, a merging radio galaxy containing an optical type I active galactic nuclei (AGN). This discovery was made through observations conducted by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) using redshifted 21-cm absorption. The outflow exhibits a blueshifted velocity likely up to with respect to the systemic velocity of the host galaxy with an absorption strength of corresponding to an optical depth of 0.002 at . The mass outflow rate ranges between and , implying an energy outflow rate ranging between and , assuming 100 K 1000 K. Plausible drivers of the outflow include…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research · Galaxies: Formation, Evolution, Phenomena
