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Cool outflows in galaxies and their implications
Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
The origin of radio emission from radio-quiet active galactic nuclei
The central nuclei of galaxies, where supermassive black holes (SMBHs) are thought to
reside, can experience phases of activity when they become active galactic nuclei (AGNs) …
reside, can experience phases of activity when they become active galactic nuclei (AGNs) …
AGN wind scaling relations and the co-evolution of black holes and galaxies
Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …
the main mechanism responsible for regulating star formation in active galactic nucleus …
Bubbles and outflows: The novel JWST/NIRSpec view of the z= 1.59 obscured quasar XID2028
Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench
star formation in galaxies, although direct observational evidence is still scarce and debated …
star formation in galaxies, although direct observational evidence is still scarce and debated …
Ionized outflows from active galactic nuclei as the essential elements of feedback
S Laha, CS Reynolds, J Reeves, G Kriss… - Nature …, 2021 - nature.com
Outflows from active galactic nuclei (AGNs) are one of the fundamental mechanisms by
which the central supermassive black hole interacts with its host galaxy. Detected in≥ 50 …
which the central supermassive black hole interacts with its host galaxy. Detected in≥ 50 …
A quasar-galaxy merger at z∼ 6.2: Black hole mass and quasar properties from the NIRSpec spectrum
We present JWST/NIRSpec integral field data of the quasar PJ308-21 at z= 6.2342. As
shown by previous ALMA and HST imaging, the quasar has two companion sources …
shown by previous ALMA and HST imaging, the quasar has two companion sources …
Gravitational torque-driven black hole growth and feedback in cosmological simulations
We investigate black hole–host galaxy scaling relations in cosmological simulations with a
self-consistent black hole growth and feedback model. Our sub-grid accretion model …
self-consistent black hole growth and feedback model. Our sub-grid accretion model …
A global view of the inner accretion and ejection flow around super massive black holes-Radiation-driven accretion disk winds in a physical context
Context. Understanding the physics and geometry of accretion and ejection around super
massive black holes (SMBHs) is important to understand the evolution of active galactic …
massive black holes (SMBHs) is important to understand the evolution of active galactic …
The size-luminosity relation of local active galactic nuclei from interferometric observations of the broad-line region
By using the GRAVITY instrument with the near-infrared (NIR) Very Large Telescope
Interferometer (VLTI), the structure of the broad (emission-) line region (BLR) in active …
Interferometer (VLTI), the structure of the broad (emission-) line region (BLR) in active …
The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflow
Mrk 231 is a nearby ultra-luminous IR galaxy exhibiting a kpc-scale, multi-phase AGN-driven
outflow. This galaxy represents the best target to investigate in detail the morphology and …
outflow. This galaxy represents the best target to investigate in detail the morphology and …