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相关论文: The Prevalence of Gas Outflows in Type 2 AGNs

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We present a systematic study of ionized gas outflows based on the velocity shift and dispersion of the [O III] {\lambda}5007 $\AA$ emission line, using a sample of ~ 5000 Type 1 AGNs at z < 0.3 selected from Sloan Digital Sky Survey. This…

星系天体物理 · 物理学 2018-09-26 Suvendu Rakshit , Jong-Hak Woo

We present gas kinematics based on the [OIII] $\lambda$5007 line and their connection to galaxy gravitational potential, active galactic nucleus (AGN) energetics, and star formation, using a large sample of ~110,000 AGNs and star-forming…

星系天体物理 · 物理学 2017-05-03 Jong-Hak Woo , Donghoon Son , Hyun-Jin Bae

We explore the relationship between the ionized gas outflows and radio activity using a sample of $\sim$ 6000 AGNs at z < 0.4 with the kinematical measurement based on the [O III] line profile and the radio detection in the VLA FIRST…

星系天体物理 · 物理学 2023-06-23 Ashraf Ayubinia , Jong-Hak Woo , Suvendu Rakshit , Donghoon Son

Energetic ionized gas outflows driven by active galactic nuclei (AGN) have been studied as a key phenomenon related to AGN feedback. To probe the kinematics of the gas in the narrow line region, [O III] ${\lambda}$5007 has been utilized in…

星系天体物理 · 物理学 2017-08-22 Daeun Kang , Jong-Hak Woo , Hyun-Jin Bae

We perform a census of ionized gas outflows using a sample of ~23,000 type 2 active galactic nuclei (AGNs) out to z~0.1. By measuring the velocity offset of narrow emission lines, i.e., [O III] {\lambda}5007 and H{\alpha}, with respect to…

星系天体物理 · 物理学 2014-10-14 Hyun-Jin Bae , Jong-Hak Woo

We present 3D models of biconical outflows combined with a thin dust plane for investigating the physical properties of the ionized gas outflows and their effect on the observed gas kinematics in type 2 active galactic nuclei (AGNs). Using…

星系天体物理 · 物理学 2016-09-20 Hyun-Jin Bae , Jong-Hak Woo

We investigate the ionized gas kinematics relationship with X-ray, radio and accreting properties using a sample of 348 nearby ($z < 0.4$) SDSS-FIRST-X-ray detected AGNs. X-ray properties of our sample are obtained from XMM-$Newton$,…

We present a detailed study of ionized outflows in a large sample of ~650 hard X-ray detected AGN. Using optical spectroscopy from the BAT AGN Spectroscopic Survey (BASS) we are able to reveal the faint wings of the [OIII] emission lines…

To investigate the connection between radio activity and AGN outflows, we present a study of ionized gas kinematics based on [O III] $\lambda$5007 emission line along the large-scale radio jet for six radio AGNs. These AGNs are selected…

星系天体物理 · 物理学 2017-12-20 Huynh Anh N. Le , Jong-Hak Woo , Donghoon Son , Marios Karouzos , Aeree Chung , Taehyun Jung , Evangelia Tremou

To investigate AGN outflows as a tracer of AGN feedback on star-formation, we perform integral-field spectroscopy of 20 type 2 AGNs at z<0.1, which are luminous AGNs with the [O III] luminosity >10$^{41.5}$ erg/s, and exhibit strong outflow…

星系天体物理 · 物理学 2017-03-15 Hyun-Jin Bae , Jong-Hak Woo , Marios Karouzos , Elena Gallo , Helene Flohic , Yue Shen , Suk-Jin Yoon

We investigate the connection between ionized gas outflows and star formation activity using a large sample of type 1 and 2 AGNs with far-IR detections or star formation rate (SFR) estimates. The strength of ionized gas outflows, measured…

星系天体物理 · 物理学 2020-09-30 Jong-Hak Woo , Donghoon Son , Suvendu Rakshit

Ionised gas kinematics provide crucial evidence of the impact that active galactic nuclei (AGN) have in regulating star formation in their host galaxies. Although the presence of outflows in AGN host galaxies has been firmly established,…

AGN-driven outflows are considered as one of the processes driving the co-evolution of supermassive black holes with their host galaxies. We present integral field spectroscopy of six Type 2 AGNs at z < 0.1, which are selected as AGNs…

星系天体物理 · 物理学 2019-04-03 Rongxin Luo , Jong-Hak Woo , Jaejin Shin , Daeun Kang , Hyun-Jin Bae , Marios Karouzos

We present the study of the gas kinematics in narrow-line regions (NLRs) of 2,009 type-2 AGNs at $z<0.34$. We construct the [O III]$\lambda$5007 emission-line images using publicly available broadband images from the Sloan Digital Sky…

星系天体物理 · 物理学 2025-05-07 Kantapon Jensangjun , Suraphong Yuma

We search type 1 AGNs among emission-line galaxies, that are typically classified as type 2 AGNs based on emission line flux ratios if a broad component in the H$\alpha$ line profile is not properly investigated. Using ~24,000 type 2 AGNs…

星系天体物理 · 物理学 2017-06-21 Da-In Eun , Jong-Hak Woo , Hyun-Jin Bae

We present spatially resolved gas kinematics, ionization, and energetics of 11 type 1 and 5 type 2 active galactic nuclei (AGNs) with strong ionized gas outflows at z $<0.3$ using Gemini Multi-Object Spectrograph Integral Field Unit…

星系天体物理 · 物理学 2023-10-13 Changseok Kim , Jong-Hak Woo , Rongxin Luo , Aeree Chung , Junhyun Baek , Huynh Anh N. Le , Donghoon Son

Outflows have been shown to be prevalent in galaxies hosting luminous active galactic nuclei (AGNs) and present a physically plausible way to couple the AGN energy output with the interstellar medium of their hosts. Despite their…

星系天体物理 · 物理学 2016-12-21 Marios Karouzos , Jong-Hak Woo , Hyun-Jin Bae

Outflows driven by active galactic nuclei (AGNs) are often invoked as agents of the long-sought AGN feedback. Yet, characterizing and quantifying the impact on their host galaxies has been challenging. We present Gemini Multi-Object…

星系天体物理 · 物理学 2016-03-23 Marios Karouzos , Jong-Hak Woo , Hyun-Jin Bae

Fast and energetic winds are invoked by galaxy formation models as essential processes in the evolution of galaxies. These outflows can be powered either by star-formation and/or AGN activity, but the relative dominance of the two…

We combine ionized gas ([N II] 6583) and stellar central velocity dispersions for a sample of 345 galaxies, with and without active galactic nuclei (AGNs), to study the dynamical state of the nuclear gas and its physical origin. The gas…

星系天体物理 · 物理学 2009-07-17 Luis C. Ho
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