430 citations · 7.5k across the 119 of their papers we have counts for
12 papers · 1 filter
The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium
H. -Y. K. Yang, M. Gaspari, C. Marlow
Feeding and feedback of active galactic nuclei (AGN) are critical for understanding the dynamics and thermodynamics of the intracluster medium (ICM) within the cores of galaxy clus…
Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
E. Cucchetti, E. Pointecouteau, P. Peille +14
Answers to the metal production of the Universe can be found in galaxy clusters, notably within their Intra-Cluster Medium (ICM). The X-ray Integral Field Unit (X-IFU) on board the…
Cooling in the X-ray halo of the rotating, massive early-type galaxy NGC 7049
A. Juráňová, N. Werner, M. Gaspari +9
The relative importance of the physical processes shaping the thermodynamics of the hot gas permeating rotating, massive early-type galaxies is expected to be different from that i…
A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
Grant R. Tremblay, Françoise Combes, J. B. Raymond Oonk +36
We present ALMA and MUSE observations of the Brightest Cluster Galaxy in Abell 2597, a nearby (z=0.0821) cool core cluster of galaxies. The data map the kinematics of a three billi…
AGN Feedback in Galaxy Group 3C 88: Cavities, Shock and Jet Reorientation
Wenhao Liu, Ming Sun, Paul Nulsen +7
We present results from the deep Chandra observation (105 ksec), together with new Giant Metrewave Radio Telescope and Very Large Array data of the AGN outburst in the radio-loud g…
Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion
Qirong Zhu, Dandan Xu, Massimo Gaspari +13
The galaxy Malin 1 contains the largest stellar disk known but the formation mechanism of this structure has been elusive. In this paper, we report a Malin 1 analogue in the 100 Mp…
Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample
V. Ghirardini, D. Eckert, S. Ettori +10
The hot plasma in galaxy clusters is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode informati…
Non-thermal pressure support in X-COP galaxy clusters
D. Eckert, V. Ghirardini, S. Ettori +13
Galaxy clusters are the endpoints of structure formation and are continuously growing through the merging and accretion of smaller structures. Numerical simulations predict that a…
X-Ray Properties of AGN in Brightest Cluster Galaxies. I.A Systematic Study of the Chandra Archive in the and Redshift Range
Lilan Yang, Paolo Tozzi, Heng Yu +5
We present a search for nuclear X-ray emission in the brightest cluster galaxies (BCGs) of a sample of groups and clusters of galaxies extracted from the Chandra archive. The exqui…
Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
M. McDonald, M. Gaspari, B. R. McNamara +1
We present a study of 107 galaxies, groups, and clusters spanning ~3 orders of magnitude in mass, ~5 orders of magnitude in central galaxy star formation rate (SFR), ~4 orders of m…
Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
Nhut Truong, Elena Rasia, Veronica Biffi +7
Recent X-ray observations of galaxy clusters show that the distribution of intra-cluster medium (ICM) metallicity is remarkably uniform in space and time. In this paper, we analyse…
The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
Veronica Biffi, Susana Planelles, Stefano Borgani +4
The uniformity of the intra-cluster medium (ICM) enrichment level in the outskirts of nearby galaxy clusters suggests that chemical elements were deposited and widely spread into t…