Ram pressure strip** in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
The Dawes Review 9: The role of cold gas strip** on the star formation quenching of satellite galaxies
L Cortese, B Catinella, R Smith - Publications of the Astronomical …, 2021 - cambridge.org
One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …
WALLABY – an SKA Pathfinder H i survey
Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
Introducing the TNG-Cluster simulation: Overview and the physical properties of the gaseous intracluster medium
We introduce the new TNG-Cluster project, an addition to the IllustrisTNG suite of
cosmological magnetohydrodynamical simulations of galaxy formation. Our objective is to …
cosmological magnetohydrodynamical simulations of galaxy formation. Our objective is to …
Jellyfish galaxies with the IllustrisTNG simulations–I. Gas-strip** phenomena in the full cosmological context
K Yun, A Pillepich, E Zinger, D Nelson… - Monthly Notices of …, 2019 - academic.oup.com
We use the IllustrisTNG simulations to study the demographics and properties of jellyfish
galaxies in the full cosmological context. By jellyfish galaxies, we mean satellites orbiting in …
galaxies in the full cosmological context. By jellyfish galaxies, we mean satellites orbiting in …
LoTSS jellyfish galaxies-I. Radio tails in low redshift clusters
ID Roberts, RJ Van Weeren, SL McGee… - Astronomy & …, 2021 - aanda.org
Context. The cluster environment has a strong impact on galaxy star formation, as seen by
the fact that clusters host proportionally more red, passive galaxies relative to the field. Ram …
the fact that clusters host proportionally more red, passive galaxies relative to the field. Ram …
Exploring the AGN–Ram Pressure Strip** Connection in Local Clusters
Ram pressure strip** (RPS) by the intracluster medium is one of the most advocated
mechanisms that affect the properties of cluster galaxies. A recent study based on a small …
mechanisms that affect the properties of cluster galaxies. A recent study based on a small …
GASP XIII. Star formation in gas outside galaxies
Based on MUSE data from the GASP survey, we study the-emitting extraplanar tails of 16
cluster galaxies at z∼ 0.05 undergoing ram pressure strip**. We demonstrate that the …
cluster galaxies at z∼ 0.05 undergoing ram pressure strip**. We demonstrate that the …
Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
We investigate the influence of environment on the cold-gas properties of galaxies at= 0
within the TNG100 cosmological, magnetohydrodynamic simulation, part of the IllustrisTNG …
within the TNG100 cosmological, magnetohydrodynamic simulation, part of the IllustrisTNG …
[HTML][HTML] The resolved scaling relations in DustPedia: Zooming in on the local Universe
Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …