Discovery of extreme [O iii] λ5007 Å outflows in high-redshift red quasars
NL Zakamska, F Hamann, I Pâris… - Monthly Notices of …, 2016 - academic.oup.com
Black hole feedback is now a standard component of galaxy formation models. These
models predict that the impact of black hole activity on its host galaxy likely peaked at z= 2 …
models predict that the impact of black hole activity on its host galaxy likely peaked at z= 2 …
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 …
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 …
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 …
The Athena x-ray integral field unit (X-IFU)
D Barret, TL Trong, JW Den Herder… - … 2016: Ultraviolet to …, 2016 - spiedigitallibrary.org
The X-ray Integral Field Unit (X-IFU) on board the Advanced Telescope for High-ENergy
Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy …
Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy …
Powerful outflows and feedback from active galactic nuclei
A King, K Pounds - Annual Review of Astronomy and …, 2015 - annualreviews.org
Active galactic nuclei (AGNs) represent the growth phases of the supermassive black holes
in the center of almost every galaxy. Powerful, highly ionized winds, with velocities∼ 0.1–0.2 …
in the center of almost every galaxy. Powerful, highly ionized winds, with velocities∼ 0.1–0.2 …
Discovery of an enormous Lyα Nebula in a massive galaxy overdensity at z= 2.3
Abstract Enormous Lyα nebulae (ELANe), unique tracers of galaxy density peaks, are
predicted to lie at the nodes and intersections of cosmic filamentary structures. Previous …
predicted to lie at the nodes and intersections of cosmic filamentary structures. Previous …
Molecular outflows in local ULIRGs: energetics from multitransition OH analysis
E González-Alfonso, J Fischer… - The Astrophysical …, 2017 - iopscience.iop.org
We report on the energetics of molecular outflows in 14 local ultraluminous infrared galaxies
(ULIRGs) that show unambiguous outflow signatures (P Cygni profiles or high-velocity …
(ULIRGs) that show unambiguous outflow signatures (P Cygni profiles or high-velocity …
Supermassive Black Hole Winds in X-rays: SUBWAYS-I. Ultra-fast outflows in quasars beyond the local Universe
We present a new X-ray spectroscopic study of 22 luminous (2× 10 45≲ L bol/erg s− 1≲ 2×
10 46) active galactic nuclei (AGNs) at intermediate redshifts (0.1≲ z≲ 0.4), as part of the …
10 46) active galactic nuclei (AGNs) at intermediate redshifts (0.1≲ z≲ 0.4), as part of the …
Quasar feedback in the ultraluminous infrared galaxy F11119+ 3257: connecting the accretion disk wind with the large-scale molecular outflow
In Tombesi et al., we reported the first direct evidence for a quasar accretion disk wind
driving a massive (> 100 M⊙ yr− 1) molecular outflow. The target was F11119+ 3257, an …
driving a massive (> 100 M⊙ yr− 1) molecular outflow. The target was F11119+ 3257, an …