Intracluster medium through three years of WMAP [PDF]
New Astronomy Reviews, 2006 9 pages and 4 figures; Proceedings of the Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006, to be published in New Astronomy ...
Niayesh Afshordi
core +7 more sources
A Multiphase Model for the Intracluster Medium [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 Nine pages, submitted to Monthly Notices of the RAS.
Daisuke Nagai +2 more
core +8 more sources
Missing thermal energy of the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2007 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,
Niayesh Afshordi +3 more
core +6 more sources
Plasma 2020 - Intracluster Medium Plasmas [PDF]
, 2019 Galaxy clusters are the largest and most massive bound objects resulting from cosmic hierarchical structure formation. Baryons account for somewhat more than 10% of that mass, with roughly 90% of the baryonic matter distributed throughout the clusters as hot ($T>1$ keV), high-$ $, very weakly collisional plasma; the so-called "intracluster medium" (
Damiano Caprioli +8 more
core +9 more sources
EDA Complex-Driven Desaturation of Heterocyclic Carbonyl Compounds Enabled by HFIP. [PDF]
Angew Chem Int Ed EnglIn this work, we report a novel light‐mediated desaturation strategy enabled by electron donor–acceptor complex formation. DFT and mechanistic studies reveal that the reaction proceeds via single‐electron transfer, hydrogen atom transfer, and base‐mediated deprotonation sequentially with pyridinium salt serving dually as oxidant and base, and ...
Maiti R +6 more
europepmc +3 more sources
Plasma Physics of the Intracluster Medium [PDF]
, 2022 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
Matthew W. Kunz +2 more
openalex +3 more sources
Modified Entropy Models for the Intracluster Medium [PDF]
The Astrophysical Journal, 2002 Accepted to ApJ (24 pages, 31 figures)
G. Mark Voit +3 more
openalex +3 more sources
Quasar Feedback on the Intracluster Medium [PDF]
The Astrophysical Journal, 2002 Galaxy groups are quite underluminous in X-rays compared to clusters, so the intracluster medium (ICM) has to be considerably underdense in the former. We consider this to be due to substantial energy fed back into the ICM when the baryons in the member galaxies condense into stars ending up in supernovae (SNe) or accrete onto central supermassive ...
A. Cavaliere, Andrea Lapi, N. Menci
+7 more sources
Altered Functional Specialization and Interhemispheric Coordination in Rhegmatogenous Retinal Detachment: Associations With Gene Expression, Neurotransmitter Receptor Distribution, and SVM-SHAP Classification: A Multimodal Neuroimaging-Transcriptomics Study Integrating Functional Metrics and Interpretable Machine Learning. [PDF]
CNS Neurosci TherAutonomy Index (AI) and Connective Flexibility of Homotopic voxels (CFH) were derived from resting‐state fMRI data following standard preprocessing. These functional metrics were computed based on the AAL90 atlas to characterize intrinsic activity and interhemispheric coordination patterns in RRD patients.
Ji Y, Wang YY, Wu XR.
europepmc +2 more sources
oMEGACat. VII. Tracing Interstellar and Intracluster Medium of ω Centauri Using Sodium Absorptions
The Astrophysical JournalWe investigate the foreground interstellar medium along the line of sight and intracluster medium of ω Centauri ( ω Cen) by measuring the equivalent width of Na I D absorptions from MUSE observations. The large line-of-sight velocity difference between ω
Z. Wang +16 more
doaj +2 more sources