Results 121 to 130 of about 1,810 (225)
In order to examine where, how and why the quenching of star formation begins in the outskirts of galaxy clusters, we investigate the de-projected radial distribution of a large sample of quenched and star-forming galaxies (SFGs) out to 30R500 around ...
De Vos, K. +5 more
core +1 more source
Survey on Visualization of Information Diffusion over Networks
Abstract Information Diffusion (ID) describes how a value (e.g., a pathogen, a rumor, a packet) spreads through an underlying “medium” network of elements (e.g., a social or computer network). Understanding the information diffusion process is essential to predicting trends, controlling misinformation, and enhancing decision‐making as well as ...
T. Baumgartl +8 more
wiley +1 more source
Massive Star Clusters in Dwarf Galaxies
Dwarf galaxies can have very high globular cluster specific frequencies, and the GCs are in general significantly more metal-poor than the bulk of the field stars. In some dwarfs, such as Fornax, WLM, and IKN, the fraction of metal-poor stars that belong
Søren S. Larsen
core +1 more source
Constraining ΛLTB models with galaxy cluster counts from next-generation surveys
Context. The Universe’s assumed homogeneity and isotropy is known as the cosmological principle. It is one of the assumptions that led to the Friedmann-Lemaître-Robertson-Walker (FLRW) metric and is a cornerstone of modern cosmology, because the metric plays a crucial role in the determination of the cosmological observables.
Z. Sakr +9 more
openaire +5 more sources
Polyamine metabolism is innervation responsive and involved in denervation‐induced muscle atrophy. Inhibition of polyamine metabolism attenuates muscle atrophy by restraining proteolysis and preserving MuSCs homeostasis. Denervation‐induced activation of FAP‐derived FGF7 drives premature MuSCs activation, while DFMO suppresses this paracrine cue to ...
Mingming Zhang +9 more
wiley +1 more source
Estimating the Mass of Galactic Components Using Machine Learning Algorithms
The estimation of galactic component masses can be carried out through various approaches that involve a host of assumptions about baryon dynamics or the dark matter model. In contrast, this work introduces an alternative method for predicting the masses
Ana A. Avilez-López +3 more
core +1 more source
An Alien Word? Cosmic Salvation within a Rahnerian Framework
Abstract The possibility of life beyond our planet raises serious theological questions for Christians, particularly in the realm of soteriology. How would Jesus of Nazareth relate to such creatures? Is he the ‘universal’ saviour, in the cosmic sense? Or are there other incarnations of the Logos, the Word or Son of God?
Brandon R. Peterson
wiley +1 more source
The chemical history of star-forming galaxies in nearby clusters [PDF]
The aim of this thesis is to investigate the influence of environment on the chemical history of star-forming galaxies in a sample of local Universe clusters.
Petropoulou, Vasiliki
core
Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments
International audienceGalaxy clusters are connected at their peripheries to the large-scale structures by cosmic filaments that funnel accreting material.
N. Aghanim +7 more
core +1 more source
ABSTRACT Aim To summarize the current evidence on reducing loneliness among informal caregivers of people with dementia, such as family members or friends. Design A systematic review. Methods The methodological quality was evaluated using the revised Cochrane risk‐of‐bias tool for randomized controlled trials and the revised JBI critical appraisal ...
Tianxue Hou +5 more
wiley +1 more source

