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 coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary universe
TM Heckman, PN Best - Annual Review of Astronomy and …, 2014 - annualreviews.org
We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …
physics and phenomenology of the processes that link the formation and evolution of …
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 …
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 …
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 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 …
The Herschel Comprehensive (U) LIRG emission survey (HERCULES): CO ladders, fine structure lines, and neutral gas cooling
MJF Rosenberg, PP Van Der Werf, S Aalto… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT (Ultra) luminous infrared galaxies ((U) LIRGs) are objects characterized by their
extreme infrared (8–1000 μm) luminosities (L LIRG> 10 11 L☉ and L ULIRG> 10 12 L☉) …
extreme infrared (8–1000 μm) luminosities (L LIRG> 10 11 L☉ and L ULIRG> 10 12 L☉) …
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 …
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 …
Star formation and nuclear activity in luminous infrared galaxies: an infrared through radio review
M Perez-Torres, S Mattila, A Alonso-Herrero… - The Astronomy and …, 2021 - Springer
Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …
studies of the interstellar medium, star formation and nuclear activity across a broad range of …