Results 151 to 160 of about 2,187 (187)

Evaluating a Digital Chronic Condition Prevention Intervention (THRIVE) in Australian General Practice: Protocol for a Mixed Methods Feasibility Study (ePREVENT-360). [PDF]

JMIR Res Protoc
Singleton G, Halcomb E, Bonney A, Hosseinzadeh H.   +3 more
europepmc   +1 more source

Determinants of skilled birth attendant delivery among reproductive age women in Lesotho: A multilevel analysis of demographic and health survey data. [PDF]

PLoS One
Endale HT, Asefa T, Mengstie TA, Getnet M, Endalew HL, Getahun AB, Dessie G, Yewodiaw TK, Enyew EF.   +8 more
europepmc   +1 more source

Evaluation of the accuracy of cone beam computed tomography (CBCT) in the detection of peri-implant fenestration. [PDF]

BMC Oral Health
Gholampour A, Mollaei M, Ehsani H, Ghobadi F, Hosseinnataj A, Yazdani M.   +5 more
europepmc   +1 more source

Two K2P Channels, TWK-46 and TWK-26 do not affect C. elegans Egg-Laying Behavior. [PDF]

MicroPubl Biol
Chen L, Beets I, Schafer W.
europepmc   +1 more source

A dual role for CTCF in development

Alonso Saiz N, Martinovic M, Rubio M, Samal P, Giselbrecht S, Braccioli L, de Wit E.   +6 more
europepmc   +1 more source

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Metals in the intracluster medium

AIP Conference Proceedings, 2012
We derived radial abundance profiles of O, Mg, Si, S and Fe in the intracluster medium (ICM) of several clusters and groups of galaxies up to about 0.3 r180 with Suzaku and those of Fe in 28 nearby brightest clusters of galaxies up to 0.3-0.5 r180 with XMM. Within 0.05 r180, Fe abundance scatters from 0.5 to 1 solar.
Kyoko Matsushita, Kosuke Sato, Eri Sakuma, Takayuki Tamura   +3 more
openaire   +1 more source

Turbulence in the Intracluster Medium

2014
We review our knowledge about turbulence in the intracluster medium, a very hot, dilute plasma that permeates clusters of galaxies. A thorough understanding of turbulence in the intracluster medium is crucial for the use of clusters to determine cosmological parameters.
Brüggen, M., Vazza, F.
openaire   +1 more source

The Intracluster Medium

1992
Clusters of galaxies are full of hot, diffuse plasma, with typical temperatures and electron densities of T ~ 7x107 K and n e ~ 10-3 cm-3, This intraclustermedium (ICM) produces copious X-ray emission, and typical cluster X-ray luminositiesare L x ~ 1043 - 1045 ergs s-1.
openaire   +1 more source

Nonlinear dynamo in the intracluster medium

Classical and Quantum Gravity, 2018
Abstract Hot plasma in galaxy clusters, the intracluster medium is observed to be magnetized with magnetic fields of around a μ G and the correlation scales of tens of kiloparsecs, the largest scales of the magnetic field so far observed in the Universe.
Andrey Beresnyak, Francesco Miniati
openaire   +1 more source

Imaging the Hot Intracluster Medium

1992
Clusters of galaxies contain large amounts of hot, diffuse x—ray emitting gas. Observations of this gas can be used to measure the gas mass, the cluster virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and ...
C. Jones, W. Forman
openaire   +1 more source