Results 1 to 10 of about 52,897 (69)
Intracluster Stars and the Chemical Enrichment of the Intracluster Medium [PDF]
We explore the contribution of intracluster stars (ICS) to the chemical enrichment history of the intracluster medium (ICM). In contrast to scenarios in which all the metals originate in cluster galaxies and are then transported into the ICM, intracluster stars enrich the ICM in situ, thereby contributing 100% of their supernovae ejecta directly into ...
Dennis Zaritsky+2 more
arxiv +5 more sources
Plasma physics of the intracluster medium [PDF]
This Chapter provides a brief tutorial on some aspects of plasma physics that are fundamental to understanding the dynamics and energetics of the intracluster medium (ICM). The tutorial is split into two parts: one that focuses on the thermal plasma component -- its stability, viscosity, conductivity, and ability to amplify magnetic fields to dynamical
Kunz, Matthew W.+2 more
arxiv +3 more sources
Evolution of vorticity and enstrophy in the intracluster medium [PDF]
Turbulence generated by large-scale motions during structure formation affects the evolution of the thermal and non-thermal components of the intracluster medium. As enstrophy is a measure of the magnitude of vorticity, we study the generation and evolution of turbulence by analysing the Lagrangian history of enstrophy.
Wittor, D.+3 more
arxiv +6 more sources
The Enrichment of the Intracluster Medium [PDF]
The enrichment of the intracluster medium (ICM) of galaxy clusters, within the framework of the supernovae-driven wind model for elliptical galaxies, has been considered under two extreme assumptions regarding the binding energy-mass-radius relations. Unless the binding energy at the time of wind commencement, for a given galactic mass, was a factor of
Francesca Matteucci, Brad K. Gibson
arxiv +7 more sources
DWARF GALAXIES AND THE ORIGIN OF INTRACLUSTER MEDIUM [PDF]
Following the recent suggestion that it is dwarf galaxies in clusters -- as opposed to large ellipticals -- that provide the intracluster gas, we estimate the metallicity of the intracluster medium (ICM) in such a case. We derive analytical expressions for the fraction of mass of dwarf galaxies that is ejected, and estimate the metallicity of the ...
Biman B. Nath, Masashi Chiba
arxiv +6 more sources
Relativistic hydrodynamic jets in the intracluster medium [PDF]
We have performed the first three-dimensional relativistic hydrodynamic simulations of extragalactic jets of pure leptonic and baryonic plasma compositions propagating into a hydrostatic intracluster medium environment. The numerical simulations use a general equation of state for a multi-component relativistic gas which closely reproduces the Synge ...
arxiv +5 more sources
THE ENRICHMENT OF THE INTRACLUSTER MEDIUM [PDF]
To determine the relative contributions of galactic and intracluster stars to the enrichment of the intracluster medium (ICM), we present X-ray surface brightness, temperature, and Fe abundance profiles for a set of twelve galaxy clusters for which we have extensive optical photometry.
Ann I. Zabludoff+4 more
openaire +2 more sources
THE INTRAGROUP VERSUS THE INTRACLUSTER MEDIUM [PDF]
ABSTRACT Galaxy groups differ from clusters primarily by way of their lower masses, M ∼ 1014 M ⊙ versus M ∼ 1015 M ⊙. We discuss how mass affects the thermal state of the intracluster or the intragroup medium, specifically as to their entropy levels and radial ...
Cavaliere, A.+2 more
openaire +4 more sources
A multiphase model for the intracluster medium [PDF]
Nine pages, submitted to Monthly Notices of the RAS.
August E. Evrard+3 more
openaire +4 more sources
On the helium fingers in the intracluster medium [PDF]
7 pages, 1 ...
Sagar Chakraborty+2 more
openaire +2 more sources