Simulations of ram-pressure stripping in galaxy-cluster interactions
D Steinhauser, S Schindler, V Springel - Astronomy & Astrophysics, 2016 - aanda.org
Context. Observationally, the quenching of star-forming galaxies appears to depend both on
their mass and environment. The exact cause of the environmental dependence is still …
their mass and environment. The exact cause of the environmental dependence is still …
The Three Hundred Project: the evolution of physical baryon profiles
The distribution of baryons provides a significant way to understand the formation of galaxy
clusters by revealing the details of its internal structure and changes over time. In this paper …
clusters by revealing the details of its internal structure and changes over time. In this paper …
The non-uniformity of galaxy cluster metallicity profiles
L Lovisari, TH Reiprich - Monthly Notices of the Royal …, 2019 - academic.oup.com
We study a sample of 207 nearby galaxy groups and clusters observed with XMM–Newton.
Key aspects of this sample include the large size, the high data quality, and the large …
Key aspects of this sample include the large size, the high data quality, and the large …
Abell 2384: the galaxy population of a cluster post-merger
F Pranger, A Böhm, C Ferrari, S Maurogordato… - Astronomy & …, 2014 - aanda.org
Context. We present a spectrophotometric analysis of the galaxy population in the area of
the merging cluster Abell 2384 at z= 0.094. Aims. We investigate the impact of the complex …
the merging cluster Abell 2384 at z= 0.094. Aims. We investigate the impact of the complex …
Metallic winds in dwarf galaxies
F Robles-Valdez, A Rodríguez-González… - The Astrophysical …, 2017 - iopscience.iop.org
We present results from models of galactic winds driven by energy injected from nuclear (at
the galactic center) and non-nuclear starbursts. The total energy of the starburst is provided …
the galactic center) and non-nuclear starbursts. The total energy of the starburst is provided …
[PDF][PDF] Constraining the quenching mechanisms of galaxy clusters through the evolution of stellar mass functions within GOGREEN and GCLASS
G Hewitt - 2024 - uwspace.uwaterloo.ca
We present an analysis of the stellar mass functions (SMFs) of 17 rich galaxy clusters within
the GOGREEN and GCLASS surveys in the redshift range of 0.8< z< 1.5, down to a stellar …
the GOGREEN and GCLASS surveys in the redshift range of 0.8< z< 1.5, down to a stellar …