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 …
MUSE Analysis of Gas around Galaxies (MAGG) – II: metal-enriched halo gas around z ∼ 1 galaxies
We present a study of the metal-enriched cool halo gas traced by Mg ii absorption around
228 galaxies at z∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around …
228 galaxies at z∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around …
The MeerKAT Fornax Survey-I. Survey description and first evidence of ram pressure in the Fornax galaxy cluster
P Serra, FM Maccagni, D Kleiner, D Molnár… - Astronomy & …, 2023 - aanda.org
The MeerKAT Fornax Survey maps the distribution and kinematics of atomic neutral
hydrogen gas (HI) in the nearby Fornax galaxy cluster using the MeerKAT telescope. The 12 …
hydrogen gas (HI) in the nearby Fornax galaxy cluster using the MeerKAT telescope. The 12 …
An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies
U Kuchner, R Haggar… - Monthly Notices of …, 2022 - academic.oup.com
Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic
web. As galaxies are accreted they are affected by their local environment before they enter …
web. As galaxies are accreted they are affected by their local environment before they enter …
GASP. XXI. Star formation rates in the tails of galaxies undergoing ram pressure strip**
Using MUSE observations from the GASP survey, we study 54 galaxies undergoing ram
pressure strip** (RPS) and spanning a wide range in galaxy mass and host cluster mass …
pressure strip** (RPS) and spanning a wide range in galaxy mass and host cluster mass …
GASP. XXII. The Molecular Gas Content of the JW100 Jellyfish Galaxy at z∼ 0.05: Does Ram Pressure Promote Molecular Gas Formation?
Within the GASP survey, aimed at studying the effect of ram pressure strip** on star
formation quenching in cluster galaxies, we analyze here ALMA observations of the jellyfish …
formation quenching in cluster galaxies, we analyze here ALMA observations of the jellyfish …
Highly ordered magnetic fields in the tail of the jellyfish galaxy JO206
A Müller, BM Poggianti, C Pfrommer, B Adebahr… - Nature …, 2021 - nature.com
Jellyfish galaxies have long tails of gas that is stripped from the disk by ram pressure due to
the motion of galaxies in the intracluster medium in galaxy clusters. Here, we present the …
the motion of galaxies in the intracluster medium in galaxy clusters. Here, we present the …
It's Cloud's illusions I recall: mixing drives the acceleration of clouds from ram pressure stripped galaxies
Ram pressure strip** can remove gas from satellite galaxies in clusters via a direct
interaction between the intracluster medium (ICM) and the interstellar medium. This …
interaction between the intracluster medium (ICM) and the interstellar medium. This …
3D Modeling of the Molecular Gas Kinematics in Optically Selected Jellyfish Galaxies
Cluster galaxies are subject to the ram pressure exerted by the intracluster medium, which
can perturb or even strip away their gas while leaving the stars undisturbed. We model the …
can perturb or even strip away their gas while leaving the stars undisturbed. We model the …