Results 31 to 40 of about 2,187 (187)
Intracluster Stars and the Chemical Enrichment of the Intracluster Medium
5 pages, accepted for publication by ApJ Letters. Changed title to follow ApJL convention, added references, and incorporated referee's comments.
Zaritsky, Dennis +2 more
openaire +2 more sources
AN ATTRACTOR FOR THE DYNAMICAL STATE OF THE INTRACLUSTER MEDIUM [PDF]
Galaxy clusters provide us with important information about the cosmology of our universe. Observations of the X-ray radiation or of the SZ effect allow us to measure the density and temperature of the hot intergalactic medium between the galaxies in a cluster, which then allow us to calculate the total mass of the galaxy cluster.
Juncher, Diana +2 more
openaire +3 more sources
A Two‐Temperature Model of the Intracluster Medium [PDF]
We investigate evolution of the intracluster medium (ICM), considering the relaxation process between the ions and electrons. According to the standard scenario of structure formation, ICM is heated by the shock in the accretion flow to the gravitational potential well of the dark halo.
openaire +2 more sources
Stability analysis of convection in the intracluster medium [PDF]
We use the machinery usually employed for studying the onset of Rayleigh--Bénard convection in hydro- and magnetohydro-dynamic settings to address the onset of convection induced by the magnetothermal instability and the heat-flux-buoyancy-driven-instability in the weakly-collisional magnetized plasma permeating the intracluster medium.
Gupta, H. +3 more
openaire +3 more sources
INTRACLUSTER MEDIUM REHEATING BY RELATIVISTIC JETS [PDF]
Accepted for publication in ...
Perucho, Manel +2 more
openaire +2 more sources
Power spectrum estimation methods on intracluster medium surface brightness fluctuations [PDF]
Accurate estimation of galaxy cluster masses is a central problem in cosmology. Turbulence is believed to introduce significant deviations from the hydrostatic mass estimates.
Bishop M. +3 more
doaj +1 more source
Missing thermal energy of the intracluster medium [PDF]
The Sunyaev-Zel'dovich (SZ) effect is a direct probe of thermal energy content of the Universe, induced in the cosmic microwave background (CMB) sky through scattering of CMB photons off hot electrons in the intracluster medium (ICM). We report a 9-sigma detection of the SZ signal in the CMB maps of Wilkinson Microwave Anisotropy Probe (WMAP) 3yr data,
Afshordi, Niayesh +3 more
openaire +3 more sources
Heating of the intracluster medium
The gravitational interaction of the system of galaxies and the ICM are treated by fluctuation theory. Fluctuation theory seems to be more adequate to describe the gravitational interaction than local theories used up to now, because gravitation is a long-range force.
A. Just +4 more
openaire +1 more source
Formation of multiphase plasma in galactic haloes and an analogy to solar plasma
Thermal instability (TI) potentially explains the origin of cold gas in the intracluster medium (ICM), which is heated sufficiently by AGN feedback. The Hα filaments seen in cluster cores provide strong motivation for TI.
Prakriti Pal Choudhury
doaj +1 more source
Understanding shape and centroid deviations in 39 strong lensing galaxy clusters in various dynamical states [PDF]
Through observational tests of strong lensing galaxy clusters, we can test simulation derived structure predictions that follow from Λ Cold Dark Matter (ΛCDM) cosmology.
Gassis Raven +10 more
doaj +1 more source

