Results 111 to 120 of about 5,809 (203)
The origin of gas stripping of galaxies in group environments
We investigate how low-mass group environments (Mvir ∼ 1012 − 13 M⊙) influence the gas content of their satellite galaxies with M* > 107 M⊙ using the NEWHORIZON2 simulation.
Rhee Jinsu +14 more
doaj +1 more source
Satellite galaxies can be used to indicate the dynamic mass of galaxy groups and clusters. In this study, we apply the axisymmetric Jeans Anisotropic Multi-Gaussian Expansion ( JAM ) modeling to satellite galaxies in 28 galaxy clusters selected from the ...
Rui Shi +9 more
doaj +1 more source
Decoding AGN Feedback with X-arithmetic: From Morphology to Physical Mechanisms
Feedback from active galactic nuclei is a key process in the evolution of massive halos in the Universe. New observational information on feedback is crucial for improving the implementation of the physics in numerical models.
Hannah McCall +6 more
doaj +1 more source
Unsupervised multimodal deep learning for galaxy morphology taxonomy: integrating ConvNeXtEmbeddings and morphological parameters for scalable survey science. [PDF]
Selim IM +3 more
europepmc +1 more source
Simulations of multi-phase gas in and around galaxies. [PDF]
Gronke M, E Schneider E.
europepmc +1 more source
An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth. [PDF]
Bogdán Á +3 more
europepmc +1 more source
LiraSearch-ultrafast ligand shape and electrostatic matching server. [PDF]
Montalvão RW +5 more
europepmc +1 more source
Ten common misconceptions about Galaxy (and why they are wrong!). [PDF]
Bacon WA +10 more
europepmc +1 more source
Fractal nature of galaxy clustering in the updated CfA redshift catalog. [PDF]
Macek WM, Wójcik D.
europepmc +1 more source

