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 …
Impact of supermassive black hole growth on star formation
CM Harrison - Nature Astronomy, 2017 - nature.com
Supermassive black holes are found at the centres of massive galaxies. During the growth of
these black holes they light up to become visible as active galactic nuclei (AGNs) and …
these black holes they light up to become visible as active galactic nuclei (AGNs) and …
Near infrared spectroscopy and star-formation histories of 3≤ z≤ 4 quiescent galaxies
C Schreiber, K Glazebrook, T Nanayakkara… - Astronomy & …, 2018 - aanda.org
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
The KMOS3D survey: demographics and properties of galactic outflows at z= 0.6–2.7
NMF Schreiber, H Übler, RL Davies… - The Astrophysical …, 2019 - iopscience.iop.org
We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …
Relativistic jet feedback–III. Feedback on gas discs
We study the interactions of a relativistic jet with a dense turbulent gaseous disc of radius∼
2 kpc. We have performed a suite of simulations with different mean density, jet power, and …
2 kpc. We have performed a suite of simulations with different mean density, jet power, and …
The fast molecular outflow in the Seyfert galaxy IC 5063 as seen by ALMA
R Morganti, T Oosterloo, JBR Oonk, W Frieswijk… - Astronomy & …, 2015 - aanda.org
We use high-resolution (0.5 arcsec) CO (2− 1) observations performed with the Atacama
Large Millimetre/submillimetre Array to trace the kinematics of the molecular gas in the …
Large Millimetre/submillimetre Array to trace the kinematics of the molecular gas in the …
Quasar-mode feedback in nearby type 1 quasars: ubiquitous kiloparsec-scale outflows and correlations with black hole properties
Quasar-mode Feedback in Nearby Type 1 Quasars: Ubiquitous Kiloparsec-scale Outflows and
Correlations with Black Hole Properties - IOPscience This site uses cookies. By continuing to …
Correlations with Black Hole Properties - IOPscience This site uses cookies. By continuing to …
Relativistic jet feedback in high-redshift galaxies–I. Dynamics
We present the results of 3D relativistic hydrodynamic simulations of interaction of active
galactic nucleus jets with a dense turbulent two-phase interstellar medium, which would be …
galactic nucleus jets with a dense turbulent two-phase interstellar medium, which would be …
Stellar and quasar feedback in concert: effects on AGN accretion, obscuration, and outflows
PF Hopkins, P Torrey… - Monthly Notices of …, 2016 - academic.oup.com
We study the interaction of feedback from active galactic nuclei (AGN) and a multiphase
interstellar medium (ISM), in simulations including explicit stellar feedback, multiphase …
interstellar medium (ISM), in simulations including explicit stellar feedback, multiphase …
Star formation quenching in massive galaxies
A Man, S Belli - Nature Astronomy, 2018 - nature.com
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