Results 161 to 170 of about 69,040 (190)

Personalised decision support in the management of patients with musculoskeletal pain in primary physiotherapy care: a cluster randomised controlled trial (the SupportPrim project). [PDF]

Pain
Granviken F, Meisingset I, Bach K, Bones AF, Simpson MR, Hill JC, van der Windt DA, Vasseljen O.   +7 more
europepmc   +1 more source

Psychotherapeutic treatments for depression in older adults. [PDF]

Cochrane Database Syst Rev
Ang L, Lee MS, Song E, Lee HW, Cao L, Zhang J, Wang Q, Jung J, Jang S, Gastaldon C, Reynolds CF, Cuijpers P, Patel V, Barbui C, Yao L, Papola D.   +15 more
europepmc   +1 more source

Laboratory evidence of Weibel magnetogenesis driven by temperature gradient using three-dimensional synchronous proton radiography. [PDF]

Sci Adv
Zhao Z, He S, An H, Lei Z, Xie Y, Yuan W, Jiao J, Zhou K, Zhang Y, Ye J, Xie Z, Xiong J, Fang Z, He X, Wang W, Zhou W, Zhang B, Zhu S, Qiao B.   +18 more
europepmc   +1 more source

A protocol of a randomized control trial to test the feasibility and efficacy of the EMPOWER social-emotional learning curriculum for youth aged 11-14 years in after-school settings. [PDF]

PLoS One
Balter AS, Moloney M, Ma C, Lee A, Pierre S, Parkes S, Pulat D, Racine N, Andrade BF.   +8 more
europepmc   +1 more source

Efficacy of Real-Time Feedback Exercise Therapy in Patients Following Total Hip Arthroplasty: Protocol for a Pilot Cluster-Randomized Controlled Trial.

JMIR Res Protoc
Widhalm K, Maul L, Durstberger S, Putz P, Leder-Berg S, Kainz H, Augat P.   +6 more
europepmc   +1 more source

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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   +2 more sources

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.
Kosuke Sato, Kyoko Matsushita, Takayuki Tamura, Eri Sakuma   +3 more
openaire   +2 more sources

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   +2 more sources

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 ...
W. Forman, C. Jones
openaire   +2 more sources

Evolution of Clusters and the Intracluster Medium

1993
I review observations and theoretical models of evolution of gas in clusters of galaxies. The mass of hot gas is an important component of clusters of galaxies, equalling or exceeding the total mass in galaxies in most clusters. The hot gas also traces the gravitational potential of the cluster, giving better measurements of the total mass of a cluster
openaire   +2 more sources