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20012026
most citedThe gas distribution in the outer regions of galaxy clusters

154 citations · 1.2k across the 27 of their papers we have counts for

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16 papers · 1 filter

astro-ph.CO2026

The dynamics of the Anglerfish cluster

B. Destefanis, M. Balboni, I. Bartalucci +8

Merging galaxy clusters represent the ideal laboratory to test our understanding of the large scale structure formation history and the processes involved. While many merging clust…

astro-ph.CO2025

In medio stat virtus: enrichment history in poor galaxy clusters

G. Riva, S. Ghizzardi, S. Molendi +6

The enrichment history of galaxy clusters and groups remains far from being fully understood. Recent measurements in massive clusters have revealed remarkably flat iron abundance p…

astro-ph.CO2025★ 3 cited

CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT

M. Balboni, F. Gastaldello, A. Bonafede +18

Modern radio telescopes are revolutionising our understanding of non-thermal phenomena in galaxy clusters, collecting large samples of extended sources with unprecedented sensitivi…

astro-ph.CO2025

CHEX-MATE: Scaling relations of radio halo profiles for clusters in the LoTSS DR2 area

M. Balboni, S. Ettori, F. Gastaldello +21

The thermal and non-thermal components in galaxy clusters have properties that, although shaped from different physical phenomena, can share some similarities, mainly driven by the…

astro-ph.CO2024★ 1 cited

Spherical bias on the 3D reconstruction of the ICM density profile in galaxy clusters

I. Veronesi, I. Bartalucci, E. Rasia +9

X-ray observations of galaxy clusters are routinely used to derive radial distributions of ICM thermdynamical properties such as density and temperature. However, observations allo…

astro-ph.CO2024★ 7 cited

CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime

G. Riva, G. W. Pratt, M. Rossetti +26

We characterise the entropy profiles of 32 very high mass () galaxy clusters (HIGHMz), selected from the CHEX-MATE sample, to study the intracl…

astro-ph.CO2024

PSZ2 G282.28+49.94, a recently discovered analogue of the famous Bullet Cluster

I. Bartalucci, M. Rossetti, W. Boschin +17

We present a detailed study of the gas and galaxy properties of the cluster PSZ2 G282.28+49.94 detected in the Planck all-sky survey. The intracluster medium (ICM) of this object a…

astro-ph.CO2024★ 1 cited

CHEX-MATE: A LOFAR pilot X-rayradio study on five radio halo clusters

M. Balboni, F. Gastaldello, A. Bonafede +24

The connection between the thermal and non-thermal properties in galaxy clusters hosting radio halos seems fairly well established. However, a comprehensive analysis of such a conn…

astro-ph.CO2024★ 29 cited

CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton

M. Rossetti, D. Eckert, F. Gastaldello +25

The "Cluster HEritage project with \xmm: Mass Assembly and Thermodynamics at the Endpoint of structure formation" (CHEX-MATE) is a multi-year Heritage program, to obtain homogeneou…

astro-ph.CO2017★ 125 cited

The cool core state of Planck SZ-selected clusters versus X-ray selected samples: evidence for cool core bias

M. Rossetti, F. Gastaldello, D. Eckert +4

We characterized the population of galaxy clusters detected with the SZ effect with Planck, by measuring the cool core state of the objects in a well-defined subsample of the Planc…

astro-ph.CO2016★ 113 cited

The XMM Cluster Outskirts Project (X-COP)

D. Eckert, S. Ettori, E. Pointecouteau +3

Galaxy clusters are thought to grow hierarchically through the continuous merging and accretion of smaller structures across cosmic time. In the local Universe, these phenomena are…

astro-ph.CO2015★ 106 cited

Measuring the dynamical state of Planck SZ-selected clusters: X-ray peak - BCG offset

M. Rossetti, F. Gastaldello, G. Ferioli +6

We want to characterize the dynamical state of galaxy clusters detected with the Sunyaev-Zeldovich (SZ) effect by Planck and compare them with the dynamical state of clusters selec…

astro-ph.CO2014★ 92 cited

The stripping of a galaxy group diving into the massive cluster A2142

D. Eckert, S. Molendi, M. Owers +7

Structure formation in the current Universe operates through the accretion of group-scale systems onto massive clusters. The detection and study of such accreting systems is crucia…

astro-ph.CO2013★ 96 cited

Abell 2142 at large scales: An extreme case for sloshing?

M. Rossetti, D. Eckert, S. De Grandi +4

We present results obtained with a new XMM-Newton observation of A2142, a famous textbook example of cluster with multiple cold fronts, which has been studied in detail with Chandr…

astro-ph.CO2011★ 154 cited

The gas distribution in the outer regions of galaxy clusters

D. Eckert, F. Vazza, S. Ettori +7

We present the analysis of a local (z = 0.04 - 0.2) sample of 31 galaxy clusters with the aim of measuring the density of the X-ray emitting gas in cluster outskirts. We compare ou…

astro-ph.CO2011★ 57 cited

Back and forth from cool core to non-cool core: clues from radio-halos

M. Rossetti, D. Eckert, B. M. Cavalleri +3

X-ray astronomers often divide galaxy clusters into two classes: "cool core" (CC) and "non-cool core" (NCC) objects. The origin of this dichotomy has been the subject of debate in…