The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319 [PDF]
Aims. We present the joint analysis of the X-ray and Sunyaev–Zel’dovich (SZ) signals in Abell 2319, the galaxy cluster with the highest signal-to-noise ratio in SZ Planck maps and that has been surveyed within our XMM-Newton Cluster Outskirts Project (X ...
V. Ghirardini +7 more
semanticscholar +1 more source
ABSTRACT Background Frailty is a multidimensional geriatric syndrome characterised by reduced physiological reserves. Multidomain interventions combining physical and cognitive activities show promise in delaying frailty and cognitive decline. However, existing programs often face high dropout rates due to joint discomfort and balance concerns among ...
Ayuto Kodama +7 more
wiley +1 more source
Forecasting Constraints from Surface Brightness Fluctuations in Galaxy Clusters
Studies of surface brightness (SB) fluctuations in the intracluster medium present an indirect estimate of turbulent pressure support and associated Mach numbers.
Charles E. Romero
doaj +1 more source
SUPPRESSION OF ELECTRON THERMAL CONDUCTION IN THE HIGH β INTRACLUSTER MEDIUM OF GALAXY CLUSTERS [PDF]
Understanding the thermodynamic state of the hot intracluster medium (ICM) in a galaxy cluster requires knowledge of the plasma transport processes, especially thermal conduction.
G. Roberg-Clark +5 more
semanticscholar +1 more source
ABSTRACT Objectives Periodontitis is a multifactorial inflammatory disease leading to the progressive destruction of the tooth‐supporting apparatus. The management of residual periodontal pockets remains a challenge for Step 3 periodontal therapy.
King‐Lun Dominic Ho +4 more
wiley +1 more source
Simulating the Arrival of the Southern Substructure in the Galaxy Cluster Abell 1758
Abell 1758 ( z ∼ 0.278) is a galaxy cluster composed of two structures, A1758N and A1758S, separated by ∼2.2 Mpc. The northern cluster is itself a dissociative merging cluster that has already been modeled by dedicated simulations.
Rubens E. G. Machado +4 more
doaj +1 more source
Quantifying the Unwinding Due to Ram Pressure Stripping in Simulated Galaxies
Galaxies moving through the gas of the intracluster medium (ICM) experience ram pressure stripping, which can leave behind a gas tail. When a disk galaxy receives the wind edge-on, however, the characteristic signature is not a typical jellyfish tail ...
Rubens E. G. Machado +2 more
doaj +1 more source
The Survival of Planetary Nebulae in the Intracluster Medium
The stellar population stripped from galaxies in clusters evolve under the extreme conditions imposed by the intracluster (IC) medium. Intracluster stars generally suffer very high systemic velocities, and evolve within a rarefied and extremely hot IC ...
Eva Villaver +4 more
core +2 more sources
Buoyant Bubbles in a Cooling Intracluster Medium I. Hydrodynamic Bubbles [PDF]
Over the past several years, numerous examples of X-ray cavities coincident with radio sources have been observed in so-called "cool core" clusters of galaxies.
Gardini, A.
core +2 more sources
Stripped Elliptical Galaxies as Probes of ICM Physics. III. Deep Chandra Observations of NGC 4552: Measuring the Viscosity of the Intracluster Medium [PDF]
We present results from a deep (200 ks) Chandra observation of the early-type galaxy NGC 4552 (M89), which is falling into the Virgo cluster. Previous shallower X-ray observations of this galaxy showed a remnant gas core, a tail to the South of the ...
R. Kraft +9 more
semanticscholar +1 more source

