Results 31 to 40 of about 476,284 (348)
Satellite Luminosities in Galaxy Groups
, 2007 Halo model interpretations of the luminosity dependence of galaxy clustering assume that there is a central galaxy in every sufficiently massive halo, and that this central galaxy is very different from all the others in the halo.
Martino, Matthew C. +2 more
core +3 more sources
The Use and Complications of Halo Gravity Traction in Children with Scoliosis
Children, 2022 Scoliosis is one of the most frequent spine deformities encountered in children and is regularly discovered after 15 years of age with a girls to boys ratio of 2:1. Vertebral arthrodesis involves both short and long term complications.
Mihai B. Popescu +4 more
doaj +1 more source
How do stars affect $\psi$DM halos?
, 2018 Wave dark matter ($\psi$DM) predicts a compact soliton core and a granular halo in every galaxy. This work presents the first simulation study of an elliptical galaxy by including both stars and $\psi$DM, focusing on the systematic changes of the central
Chan, James H. H. +3 more
core +1 more source
Preliminary Assessment of Quantitative Phase Analysis from Focal Construct Tomography
NDT - Journal of Non-Destructive TestingNew methods for real-time materials phase identification based upon focal construct tomography (FCT) have been examined. Such quantitative assessment has significant potential in sectors where in-line analysis is required, including screening within ...
Varsha Samuel +5 more
doaj +1 more source
Frontiers in Medicine, 2020 Acinetobacter baumannii is a leading cause of healthcare-associated infections worldwide. Its various intrinsic and acquired mechanisms of antibiotic resistance make the therapeutic challenge even more serious. One of the promising alternative treatments
Goran Vukotic +10 more
doaj +1 more source
The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
, 2017 Dark matter halo clustering depends not only on halo mass, but also on other properties such as concentration and shape. This phenomenon is known broadly as assembly bias.
Bosch, Frank C. van den +8 more
core +1 more source
The Identification of Dark Matter, 2007 The size and time of formation of the first gravitationally bound objects in the Universe is set by the microphysical properties of the dark matter. It is argued that observations seem to favour cold and thermal candidates for the main contribution to the dark matter.
openaire +3 more sources
Reexamination of Mysticism in the Principles of Persian Miniatures Representing Muhammad’s (P.B.U.H.) Ascension [PDF]
پیکره, 2017 One can observe many Islamic and mystic representations in Persian miniatures the most salient of which are scenes depicting the Muhammad’s (P.B.U.H.) ascension (Miraj).
Victoria Karimi, Hanieh Gheisi
doaj +1 more source
How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
, 2018 Clustering of dark matter halos has been shown to depend on halo properties beyond mass such as halo concentration, a phenomenon referred to as halo assembly bias.
Hahn, ChangHoon, Vakili, Mohammadjavad
core +1 more source
Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
, 2019 We use the UniverseMachine to analyze the source of scatter between the central galaxy mass, the total stellar mass in the halo, and the dark matter halo mass.
Behroozi, Peter +4 more
core +1 more source