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 …
AGN outflows and feedback twenty years on
It is twenty years since the seminal works by Magorrian and co-authors and by Silk and
Rees, which, along with other related work, ignited an explosion of publications connecting …
Rees, which, along with other related work, ignited an explosion of publications connecting …
Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy
Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …
but it is difficult to observe from Earth. The Herschel Space Observatory provided …
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 …
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 …
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 …
A preferential growth channel for supermassive black holes in elliptical galaxies at z≲ 2
The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …
Molecular outflows in local galaxies: Method comparison and a role of intermittent AGN driving
D Lutz, E Sturm, A Janssen, S Veilleux, S Aalto… - Astronomy & …, 2020 - aanda.org
We report new detections and limits from a NOEMA and ALMA CO (1-0) search for
molecular outflows in 13 local galaxies with high far-infrared surface brightness, and …
molecular outflows in 13 local galaxies with high far-infrared surface brightness, and …
Ionized outflows in local luminous AGN: what are the real densities and outflow rates?
We report on the determination of electron densities, and their impact on the outflow masses
and rates, measured in the central few hundred parsecs of 11 local luminous active …
and rates, measured in the central few hundred parsecs of 11 local luminous active …
Complex AGN feedback in the Teacup galaxy-A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
Context. The z∼ 0.1 type-2 QSO J1430+ 1339, known as the “Teacup”, is a complex galaxy
showing a loop of ionised gas∼ 10 kpc in diameter, co-spatial radio bubbles, a compact (∼ …
showing a loop of ionised gas∼ 10 kpc in diameter, co-spatial radio bubbles, a compact (∼ …