Results 81 to 90 of about 2,679,570 (255)
Machine Learning–Driven Insights Into the Self‐Assembly of Gold–Thiolate Nanoclusters
A machine‐learned atomistic potential, trained by data from density‐functional theory calculations on thiolate‐protected gold nanoclusters, is applied to investigate cluster–cluster reactions in 0.1 µs timescale molecular dynamics simulations. Starting from a few experimentally known cluster stoichiometries and structures, the simulations show a ...
Maryam Sabooni Asre Hazer +1 more
wiley +1 more source
XMM-Newton observation of M 87 - I. Single-phase temperature structure of intracluster medium
We report the results of a detailed analysis of the temperature structure of the X-ray emitting plasma halo of M 87, the cD galaxy of the Virgo Cluster. Using the MEKAL model, the data provide strong indications that the intracluster medium has a single ...
A. Finoguenov +7 more
core +1 more source
Multiscale analysis of turbulence evolution in the density-stratified intracluster medium [PDF]
The diffuse hot medium inside clusters of galaxies typically exhibits turbulent motions whose amplitude increases with radius, as revealed by cosmological hydrodynamical simulations. However, its physical origin remains unclear. It could either be due to
Xun Shi, D. Nagai, E. Lau
semanticscholar +1 more source
Detrending Changes the Temporal Dynamics of a Semantic Fluency Task
Objective: To study the dynamics of clustering semantic fluency responses and switching between clusters. Methods: We conducted a cross-sectional study of participants (N=60) in a study of patient reported outcomes who were given the Saint Louis ...
Steven Lenio +6 more
doaj +1 more source
Histidine Protonation and the Oxidizing Power of the Oxygen‐Evolving Complex
Protonation of D1‐His337 governs the oxidizing power of the Mn4CaO5 cluster in photosystem II. Its singly protonated form is unstable, resulting in histidine oxidation and disruption of Mn oxidation, whereas the doubly protonated form is stable and upshifts the cluster redox potential, enabling efficient water oxidation.
Keisuke Saito, Hiroshi Ishikita
wiley +1 more source
The presence of dense, neutral hydrogen clouds in the hot, diffuse intragroup and intracluster (IC) medium is an important clue to the physical processes controlling the survival of cold gas and sheds light on cosmological baryon flows in massive halos ...
Avinash Chaturvedi +6 more
doaj +1 more source
Heating and enriching the intracluster medium [PDF]
23 pages, accepted by MNRAS. Some changes in response to referee's comments.
Short, C. J. +2 more
openaire +2 more sources
On the basis of core and log data, a Bayesian‐Optimized Random Forest model achieved 92.76% accuracy in classifying tight sandstone reservoirs. A gray relational analysis‐derived evaluation index shows > 80% consistency with actual gas zones. ABSTRACT Tight sandstone gas (TSG), an unconventional oil–gas resource, has heterogeneous reservoirs ...
Yin Yuan +8 more
wiley +1 more source
Calcium-rich gap transients: solving the calcium conundrum in the intracluster medium [PDF]
X-ray measurements suggest that the abundance of calcium in the intracluster medium is higher than can be explained using favored models for core-collapse and Type Ia supernovae alone.
Kollmeier, Juna +2 more
core
A Generative Model for Realistic Galaxy Cluster X-Ray Morphologies
The X-ray morphologies of clusters of galaxies display significant variations, reflecting their dynamical histories and the nonlinear dependence of X-ray emissivity on the density of the intracluster gas. Qualitative and quantitative assessments of X-ray
Maya Benyas +4 more
doaj +1 more source

