Results 141 to 150 of about 2,662,849 (293)
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
X-ray Observations of the Chemical Abundances in the Intra-Cluster Medium
Clusters of galaxies as the largest clearly defined objects in our Universe are ideal laboratories to study the distribution of the most abundant chemical elements heavier than hydrogen and helium and the history of their production.
Böhringer, Hans
core
Supernovae Types Ia/II and Intracluster Medium Enrichment [PDF]
We re-examine the respective roles played by supernovae (SNe) Types Ia and II in enriching the intracluster medium (ICM) of galaxy clusters, in light of the recent downward shift of the ASCA abundance ratios of alpha-elements to iron favoured by Ishimaru
Gibson, Brad K. +2 more
core +2 more sources
HOW AGN JETS HEAT THE INTRACLUSTER MEDIUM—INSIGHTS FROM HYDRODYNAMIC SIMULATIONS [PDF]
Feedback from active galactic nuclei (AGNs) is believed to prevent catastrophic cooling in galaxy clusters. However, how the feedback energy is transformed into heat, and how the AGN jets heat the intracluster medium (ICM) isotropically, still remain ...
H.-Y. Karen Yang, C. Reynolds
semanticscholar +1 more source
Background Common mental disorders (CMDs) are increasingly recognized as a major public health challenge worldwide, with adolescent girls bearing a disproportionate burden. Moreover, iron deficiency (ID) and iron deficiency anemia (IDA) remain prevalent nutritional problems among adolescents.
Shemsu Kedir +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
Implications of a Nonthermal Origin of the Excess EUV Emission from the Coma Cluster of Galaxies
The inverse Compton (IC) interpretation of the excess EUV emission, that was recently reported from several clusters of galaxies, suggests that the amount of relativistic electrons in the intracluster medium is highly significant, W_e>10^{61} erg ...
A. M. Atoyan +15 more
core +2 more sources
Introducing the TNG-Cluster Simulation: overview and physical properties of the gaseous intracluster medium [PDF]
Dylan Nelson +6 more
openalex +1 more source
Objectives Irregular sleep, frequently resulting from night shifts, is associated with various mental health issues. However, the specific associations among these factors remain unclear. This study aimed to investigate the associations of night shift frequency with depressive, anxiety, and comorbid depressive–anxiety symptoms and to estimate the ...
Chenhao Zhang +10 more
wiley +1 more source
THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 < z < 1.5 [PDF]
We present the results of an X-ray spectral analysis of 153 galaxy clusters observed with the Chandra, XMM-Newton, and Suzaku space telescopes. These clusters, which span 0 < z < 1.5, were drawn from a larger, mass-selected sample of galaxy clusters ...
M. McDonald +21 more
semanticscholar +1 more source

