首页|The transition from galaxy-wide gas inflow to outflow in quasar host galaxies

The transition from galaxy-wide gas inflow to outflow in quasar host galaxies

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The transition from galaxy-wide gas inflow to outflow in quasar host galaxies
Galactic-scale outflows driven by active galactic nuclei(AGNs)represent a commonly invoked feedback mechanism within galaxy evolution models.However,the interactions among interstellar gas on galactic scales,the propagation of AGN outflows,and the fundamental parameters of AGNs during their evolutionary processes remain poorly understood.Notably,powerful nu-clear outflows are typically associated with the early stages of AGN activity,which are characterized by high accretion rates and weak narrow emission lines.In our analysis of a sample of quasars hosting Mgn narrow absorption lines(NALs)obtained from the Sloan Digital Sky Survey,we identify a previously unobserved phenomenon wherein galaxy-scale inflow transitions to outflow dominance,concurrent with a notable increase in the strength of the narrow[O Ⅲ]line,achieving a confidence level of 6.7σ.This indicates that while nuclear outflows diminish,galaxy-wide outflows intensify as AGNs evolve.These findings suggest that early-stage outflows interact with the interstellar medium on a galactic scale,thereby facilitating a gradual transition to galaxy-wide outflows.This provides observational support for the hypothetical multi-stage propagation of AGN outflows that globally regulates galaxy evolution.

active galactic nucleiquasargalaxy windsgalaxy evolutionfeedback

Zhicheng He、Zhifu Chen、Guilin Liu、Tinggui Wang、Luis C.Ho、Junxian Wang、Weihao Bian、Zheng Cai、Guobin Mou、Qiusheng Gu、Zhiwen Wang

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CAS Key Laboratory for Research in Galaxies and Cosmology,Department of Astronomy,University of Science and Technology of China,Hefei 230026,China

Department of Physics,Guangxi Minzu University Nanning 530006,China

Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China

School of Physics,Nanjing Normal University,Nanjing 210046,China

Department of Astronomy,Tsinghua University,Beijing 100084,China

School of Astronomy and Space Science,Nanjing University,Nanjing 210093,China

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active galactic nuclei quasar galaxy winds galaxy evolution feedback

2024

中国科学:物理学 力学 天文学(英文版)
中国科学院

中国科学:物理学 力学 天文学(英文版)

CSTPCD
影响因子:0.91
ISSN:1674-7348
年,卷(期):2024.67(12)