Results 21 to 30 of about 392 (130)

Simulations of AGN-driven Galactic Outflow Morphology and Content [PDF]

open access: yesAstronomical Journal, 2022
Using a series of 3D relativistic hydrodynamical simulations of active galactic nuclei (AGN) we investigate how AGN power, a clumpy interstellar medium (ISM) structure, and AGN jet angle with respect to the galactic disk affect the morphology and content
R. Tanner, K. Weaver
semanticscholar   +1 more source

DRIVING OUTFLOWS WITH RELATIVISTIC JETS AND THE DEPENDENCE OF ACTIVE GALACTIC NUCLEUS FEEDBACK EFFICIENCY ON INTERSTELLAR MEDIUM INHOMOGENEITY [PDF]

open access: yes, 2012
We examine the detailed physics of the feedback mechanism by relativistic active galactic nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc-scale core of galaxies using 29 three-dimensional grid-based ...
A. Wagner, G. Bicknell, M. Umemura
semanticscholar   +1 more source

Establishing the impact of luminous AGN with multi-wavelength observations and simulations [PDF]

open access: yesProceedings of the International Astronomical Union, 2023
Cosmological simulations fail to reproduce realistic galaxy populations without energy injection from active galactic nuclei (AGN) into the interstellar medium (ISM) and circumgalactic medium (CGM); a process called ‘AGN feedback’.
C. Harrison, A. Girdhar, S. R. Ward
semanticscholar   +1 more source

Shocks, clouds, and atomic outflows in active galactic nuclei hosting relativistic jets [PDF]

open access: yesAstronomy & Astrophysics
A number of observations have revealed atomic and/or molecular lines in active galaxies hosting jets and outflows. Line widths indicate outward motions of hundreds to a few thousands of kilometers per second.
M. Perucho
semanticscholar   +1 more source

Dents in the Veil: Protostellar feedback in Orion [PDF]

open access: yesAstronomy & Astrophysics, 2022
Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars regulate the physical and chemical composition of the interstellar medium (ISM) significantly.
Ü. Kavak   +5 more
semanticscholar   +1 more source

You Shall Not Pass! The Propagation of Low-/Moderate-powered Jets Through a Turbulent Interstellar Medium [PDF]

open access: yesAstrophysical Journal
Feedback from black-hole-powered jets has been invoked in many cosmological simulations to regulate star formation and quench galaxies. Despite this, observational evidence of how jets might be able to affect their hosts remains scarce, especially for ...
O. Borodina   +8 more
semanticscholar   +1 more source

AGN feedback compared: jets versus radiation [PDF]

open access: yes, 2017
Feedback by Active Galactic Nuclei is often divided into quasar and radio mode, powered by radiation or radio jets, respectively. Both are fundamental in galaxy evolution, especially in late-type galaxies, as shown by cosmological simulations and ...
S. Cielo   +4 more
semanticscholar   +1 more source

Connecting outflows with radio emission in active galactic nuclei at cosmic noon [PDF]

open access: yesAstronomy & Astrophysics
Active galactic nucleus (AGN) feedback is a well-known mechanism in the evolution of galaxies. However, constraining its parameters remains a significant challenge. One open question is the driving mechanism of galaxy-scale outflows.
G. S. Ilha   +19 more
semanticscholar   +1 more source

A MeerKAT view of the parsec-scale jets in the black-hole X-ray binary GRS 1758-258 [PDF]

open access: yesAstronomy & Astrophysics
Jets from accreting black-hole (BH) X-ray binary (XRB) systems are powerful outflows that release a large fraction of the accretion energy to the surrounding environment, providing a feedback mechanism that may alter the properties of the interstellar ...
I. Mariani   +7 more
semanticscholar   +1 more source

Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293 [PDF]

open access: yes, 2015
Fast outflows of gas, driven by the interaction between the radio jets and interstellar medium (ISM) of the host galaxy, are being observed in an increasing number of galaxies. One such example is the nearby radio galaxy 3C 293.
E. Mahony   +7 more
semanticscholar   +1 more source

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