Results 101 to 110 of about 16,927 (234)
Metal enrichment of the intracluster medium: SN-driven galactic winds
We investigate the role of supernova (SN)-driven galactic winds in the chemical enrichment of the intracluster medium (ICM). Such outflows on galactic scales have their origin in huge star forming regions and expel metal enriched material out of the ...
Balestra +34 more
core +1 more source
We study the global kinematics of the Perseus galaxy cluster (A426) at redshift z = 0.017 using a large sample of galaxies from our new MMT/Hectospec spectroscopic observation for this cluster.
Wooseok Kang +5 more
doaj +1 more source
On viscosity, conduction and sound waves in the intracluster medium
Recent X-ray and optical observations of the Perseus cluster indicate that the viscous and conductive dissipation of sound waves is the mechanism responsible for heating the intracluster medium and thus balancing radiative cooling of cluster cores.
A. C. Fabian +53 more
core +4 more sources
Contribution of Type Ia and Type II Supernovae to Intracluster Medium Enrichment [PDF]
Shigehiro Nagataki, Katsuhiko Sato
openalex +1 more source
We present a systematic study of the thermodynamic properties of the intracluster medium (ICM), including the plasma conditions in the ICM, in the merging galaxy cluster A3667 using Suzaku. We analyze the X-ray spectra of the ICM between the northwestern
Mona Shishido +2 more
doaj +1 more source
Constraints on Ultraviolet Absorption in the Intracluster Medium of Abell 1030 [PDF]
Anton M. Koekemoer +5 more
openalex +1 more source
On the Origin of the Ancient, Large-scale Cold Front in the Perseus Cluster of Galaxies
The intracluster medium of the Perseus Cluster exhibits spiral-shaped X-ray surface brightness discontinuities known as “cold fronts,” which simulations indicate are caused by the sloshing motion of the gas after the passage of a subcluster.
Elena Bellomi +6 more
doaj +1 more source
We present the first results of one extremely high-resolution, nonradiative magnetohydrodynamical cosmological zoom-in simulation of a massive cluster with a virial mass of M _vir = 2.0 × 10 ^15 solar masses. We adopt a mass resolution of 4 × 10 ^5 M _⊙
Ulrich P. Steinwandel +3 more
doaj +1 more source
A Prediction of Observable Rotation in the Intracluster Medium of Abell 3266 [PDF]
K. Roettiger, Ricardo A. Flores
openalex +1 more source

