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Related papers: Cold-gas outflows in typical low-redshift galaxies…

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We report on a S/N-limited search for low-ionization gas outflows in the spectra of the 0.11 < z < 0.54 objects in the EGS portion of the DEEP2 survey. Doppler shifts from the host galaxy redshifts are systematically searched for in the Na…

Astrophysics · Physics 2015-03-13 Taro Sato , Crystal L. Martin , Kai G. Noeske , David C. Koo , Jennifer M. Lotz

We perform simulations to study the effects of active galactic nuclei (AGNs) radiation and wind feedback on the properties of slowly rotating accretion flow at parsec scale. We find that when only radiative feedback is considered, outflows…

High Energy Astrophysical Phenomena · Physics 2019-09-11 De-Fu Bu , Xiao-Hong Yang

The effects of Active Galactic Nuclei (AGNs) on their host-galaxies depend on the coupling between the injected energy and the interstellar medium (ISM). Here, we model and quantify the impact of long-range AGN ionizing radiation -- in…

Astrophysics of Galaxies · Physics 2015-02-09 Orianne Roos , Stéphanie Juneau , Frédéric Bournaud , Jared M. Gabor

Despite the importance of feedback from active galactic nuclei (AGNs) in models of galaxy evolution, observational constraints on the influence of AGN feedback on star formation remain weak. To this end, we have compared the star formation…

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…

Astrophysics of Galaxies · Physics 2016-12-21 Marios Karouzos , Jong-Hak Woo , Hyun-Jin Bae

Analysis of the frequency and physical properties of galaxies with star-formation and AGN activity in different environments in the local universe is a cornerstone for understanding structure formation and galaxy evolution. We have built a…

Astrophysics · Physics 2008-11-26 Pietro Reviglio , David J. Helfand

Observations of massive outflows with detectable central AGN typically find them within radii $\lesssim 10$ kpc. We show that this apparent size restriction is a natural result of AGN driving if this process injects total energy only of…

Astrophysics of Galaxies · Physics 2016-09-21 Kastytis Zubovas , Andrew King

Feedback in massive galaxies generally involves quenching of star formation, a favored candidate being outflows from a central supermassive black hole. At high redshifts however, explanation of the huge rates of star formation often found…

Astrophysics of Galaxies · Physics 2016-01-27 Rebekka Bieri , Yohan Dubois , Joseph Silk , Gary A. Mamon

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…

Astrophysics of Galaxies · Physics 2014-10-14 Hyun-Jin Bae , Jong-Hak Woo

Observations point towards a close connection between nuclear starbursts, active galactic nuclei (AGN), and outflow phenomena. An evolutionary sequence, starting from a dust-obscured ultra-luminous infrared galaxy and eventually leading to…

Astrophysics of Galaxies · Physics 2016-10-05 W. Ishibashi , A. C. Fabian

[Abridged] Active Galactic Nuclei (AGN) are thought to be responsible for the suppression of star formation in massive ~10$^{10}$ M$_\odot$ galaxies. While this process is a key feature in numerical simulations, it is not yet unambiguously…

We present Keck/LRIS-B spectra for a sample of ten AEGIS X-ray AGN host galaxies and thirteen post-starburst galaxies from SDSS and DEEP2 at 0.2<z<0.8 in order to investigate the presence, properties, and influence of outflowing galactic…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-23 Alison L. Coil , Benjamin J. Weiner , Daniel E. Holz , Michael C. Cooper , Renbin Yan , James Aird

The role of active galactic nuclei (AGN) feedback in dwarf galaxies remains poorly understood, with conventional wisdom suggesting it primarily suppresses star formation. Using high-resolution MACER3D simulations that directly resolve the…

Astrophysics of Galaxies · Physics 2025-10-27 Tingfang Su , Suoqing Ji , Feng Yuan , Haojie Xia , Yuxuan Zou

Metals in the hot gaseous halos of galaxies encode the history of star formation as well as the feedback processes that eject metals from the galaxies. X-ray observations suggest that massive galaxies have extended distributions of metals…

Astrophysics of Galaxies · Physics 2020-11-25 Ena Choi , Ryan Brennan , Rachel S. Somerville , Jeremiah P. Ostriker , Michaela Hirschmann , Thorsten Naab

Increasing evidence shows that AGN with radio detections have more perturbed ionized gas kinematics and higher outflow detection rates, suggesting a link between radio emission and these processes. In galaxies with weak or ambiguous AGN…

Astrophysics of Galaxies · Physics 2026-03-04 Marco Albán , Dominika Wylezalek , Pranav Kukreti , Rogemar A. Riffel , Rogerio Riffel

AGN activity is known to drive fast outflows of gas. We report the discovery of fast outflows of neutral gas with velocities over 1000 km/s in a number of radio galaxies. In the best studied object, 3C~293, the kinematical properties of the…

Astrophysics · Physics 2009-11-10 T. A. Oosterloo , R. Morganti , B. H. C. Emonts , C. N. Tadhunter

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…

Astrophysics of Galaxies · Physics 2017-03-15 Hyun-Jin Bae , Jong-Hak Woo , Marios Karouzos , Elena Gallo , Helene Flohic , Yue Shen , Suk-Jin Yoon

We analyze ionized gas emission lines in deep rest-frame optical spectra of 16 quiescent galaxies at redshift $1.7<z<3.5$ observed with JWST/NIRSpec by the Blue Jay survey. Robust detection of emission lines in $75\%$ of the sample…

We investigated the influence of Active Galactic Nuclei (AGN) feedback on star formation in red spiral galaxies by analyzing a sample of 324 red and 273 blue face-on spirals selected from 115 low-redshift galaxy clusters. This…

Residual star formation at late times in early-type galaxies and their progenitors must be suppressed in order to explain the population of red, passively evolving systems we see today. Likewise, residual or newly accreted reservoirs of…

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