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 many routes to AGN feedback
R Morganti - Frontiers in Astronomy and Space Sciences, 2017 - frontiersin.org
The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds, or radio
plasma jets, is known to impact on the surrounding interstellar medium. The result of these …
plasma jets, is known to impact on the surrounding interstellar medium. The result of these …
Planck 2015 results-XX. Constraints on inflation
PAR Ade, N Aghanim, M Arnaud, F Arroja… - Astronomy & …, 2016 - aanda.org
We present the implications for cosmic inflation of the Planck measurements of the cosmic
microwave background (CMB) anisotropies in both temperature and polarization based on …
microwave background (CMB) anisotropies in both temperature and polarization based on …
Cold molecular outflows in the local Universe and their feedback effect on galaxies
We study molecular outflows in a sample of 45 local galaxies, both star forming and active
galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter …
galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter …
Massive molecular outflows and evidence for AGN feedback from CO observations
We study the properties of massive, galactic-scale outflows of molecular gas and investigate
their impact on galaxy evolution. We present new IRAM PdBI CO (1–0) observations of local …
their impact on galaxy evolution. We present new IRAM PdBI CO (1–0) observations of local …
Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
We present integral field unit observations covering the [o iii] λλ4959, 5007 and Hβ emission
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …
Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
Powerful winds driven by active galactic nuclei are often thought to affect the evolution of
both supermassive black holes and their host galaxies, quenching star formation and …
both supermassive black holes and their host galaxies, quenching star formation and …
The physics of galactic winds driven by active galactic nuclei
CA Faucher-Giguère, E Quataert - Monthly Notices of the Royal …, 2012 - academic.oup.com
Active galactic nuclei (AGN) drive fast winds in the interstellar medium of their host galaxies.
It is commonly assumed that the high ambient densities and intense radiation fields in …
It is commonly assumed that the high ambient densities and intense radiation fields in …
The KMOS3D survey: demographics and properties of galactic outflows at z= 0.6–2.7
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 …
Quasar feedback and the origin of radio emission in radio-quiet quasars
Abstract We analyse Sloan Digital Sky Survey spectra of 568 obscured luminous quasars.
The [O iii] λ5007 Å emission line shows blueshifts and blue excess, indicating that some of …
The [O iii] λ5007 Å emission line shows blueshifts and blue excess, indicating that some of …