Results 11 to 20 of about 46,933 (305)
Starbursts in multiple galaxy mergers [PDF]
We numerically investigate stellar and gaseous dynamical evolution of mergers between five identical late-type disk galaxies with the special emphasis on star formation history and chemical evolution of multiple galaxy mergers.
Athanassoula E.+9 more
core +5 more sources
Galaxy mergers in a fractal cosmology
This work discusses the influence of galaxy mergers in the evolution of a parabolic Lemaître–Tolman–Bondi (LTB) cosmology with simultaneous big bang endowed with two consecutive single fractal galaxy distributions systems possessing fractal dimension D ...
Bruno J. Souza+2 more
doaj +3 more sources
Merger relics of cluster galaxies [PDF]
Context. Sheen and collaborators recently found that a surprisingly large portion (38%) of massive early-type galaxies in heavy clusters show strong merger-related disturbed features.
Ji, Inchan+4 more
core +5 more sources
Formation of a Polar Ring Galaxy in a Galaxy Merger [PDF]
We numerically investigate stellar and gas dynamics in star-forming and dissipative galaxy mergers between two disk galaxies with specific orbital configurations. We find that violent relaxation combined with gaseous dissipation in galaxy merging transforms two disk galaxies into one S0 galaxy with polar-rings: Both the central S0-like host and the ...
Kenji Bekki
+9 more sources
Simulations of galaxy mergers [PDF]
J. V. Villumsen
openalex +3 more sources
NGC 3310, a galaxy merger? [PDF]
10 pages, 11 figures, accepted for publication in A& ...
M. Kregel, R. Sancisi
openalex +5 more sources
Jet Interaction with Galaxy Cluster Mergers
Active galactic nucleus (AGN) bubbles in cool-core galaxy clusters are believed to facilitate the transport of cosmic-ray electrons (CRe) throughout the cluster.
P. Domínguez-Fernández+6 more
doaj +3 more sources
On the dependence of galaxy morphologies on galaxy mergers [PDF]
The distribution of galaxy morphological types is a key test for models of galaxy formation and evolution, providing strong constraints on the relative contribution of different physical processes responsible for the growth of the spheroidal components.
Fabio Fontanot+8 more
openaire +4 more sources
We present the results of an Eulerian adaptive mesh refinement (AMR) hydrodynamical and N-body simulation in a $ $CDM cosmology. The simulation incorporates common cooling and heating processes for primordial gas. A specific halo finder has been designed and applied in order to extract a sample of galaxy clusters directly obtained from the simulation ...
Susana Planelles, Vicent Quilis
openaire +3 more sources
The Merger Rate of Massive Galaxies [PDF]
We calculate the projected two point correlation function for samples of luminous and massive galaxies in the COMBO-17 photometric redshift survey, focusing particularly on the amplitude of the correlation function at small projected radii and exploring the constraints such measurements can place on the galaxy merger rate.
Bell, E+5 more
openaire +4 more sources