Results 91 to 100 of about 16,803 (214)

The X-ray Luminosity - Velocity Dispersion relation in the REFLEX Cluster Survey [PDF]

open access: yes, 2003
We present an estimate of the bolometric X-ray luminosity - velocity dispersion L_x - sigma_v relation measured from a new, large and homogeneous sample of 171 low redshift, X-ray selected galaxy clusters.
A. Ortiz-Gil   +44 more
core   +3 more sources

Isomorphic Control in Energy Storage Systems Based on Graph‐Based Digital Twins

open access: yesDigital Twins and Applications, Volume 3, Issue 1, January/December 2026.
This paper proposes a graph‐based framework leveraging Activity‐on‐Edge networks to establish structural isomorphism between virtual models and physical controllers. Validated through a Mixed‐Integer Linear Programming‐based Automatic Generation Control strategy, the architecture effectively bridges the implementation gap, ensuring deterministic real ...
Zhijun Zhou   +4 more
wiley   +1 more source

Chemical Evolution Of Galaxies And Intracluster Medium [PDF]

open access: yes, 2004
In this series of lectures I discuss the basic principles and the modelling of the chemical evolution of galaxies. In particular, I present models for the chemical evolution of the Milky Way galaxy and compare them with the available observational data.
openaire   +2 more sources

Buoyancy Instabilities in a Weakly Collisional Intracluster Medium

open access: yes, 2012
The intracluster medium of galaxy clusters is a weakly collisional, high-beta plasma in which the transport of heat and momentum occurs primarily along magnetic-field lines.
Balbus   +33 more
core   +1 more source

Info‐KMeans: Enhancing Wireless Sensor Network Lifetime Through Information‐Aware Clustering

open access: yesIET Wireless Sensor Systems, Volume 16, Issue 1, January/December 2026.
This paper introduces info‐kmeans, a two‐stage wireless sensor network (WSN) protocol, that uses conditional‐entropy‐based sleep scheduling to deactivate informationally redundant nodes, then applies k‐means clustering only to the remaining information‐rich active nodes for energy‐efficient data forwarding.
Omid Abolghasemi   +2 more
wiley   +1 more source

Forecasting Constraints from Surface Brightness Fluctuations in Galaxy Clusters

open access: yesThe Astrophysical Journal
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

Quantifying the Unwinding Due to Ram Pressure Stripping in Simulated Galaxies

open access: yesGalaxies
Galaxies moving through the gas of the intracluster medium (ICM) experience ram pressure stripping, which can leave behind a gas tail. When a disk galaxy receives the wind edge-on, however, the characteristic signature is not a typical jellyfish tail ...
Rubens E. G. Machado   +2 more
doaj   +1 more source

Buoyant Bubbles in a Cooling Intracluster Medium I. Hydrodynamic Bubbles [PDF]

open access: yes, 2006
Over the past several years, numerous examples of X-ray cavities coincident with radio sources have been observed in so-called "cool core" clusters of galaxies.
Gardini, A.
core   +2 more sources

A Systematic Review of VANET Routing Protocols for Intelligent Transport Systems (ITSs)

open access: yesJournal of Advanced Transportation, Volume 2026, Issue 1, 2026.
The swift improvement of wireless communication technology has aided the creation of vehicular ad hoc networks (VANETs) as a revolutionary option for the realization of intelligent transportation systems (ITSs). VANETs facilitate seamless communication between vehicles and infrastructure (V2I) and among the vehicles themselves (V2V). These networks can
Roopa Tirumalasetti   +4 more
wiley   +1 more source

Simulating the Arrival of the Southern Substructure in the Galaxy Cluster Abell 1758

open access: yesThe Astrophysical Journal
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

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