Results 91 to 100 of about 52,179 (329)
Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
Galaxies are believed to be in one-to-one correspondence with simulated dark matter subhalos. We use high-resolution N-body simulations of cosmological volumes to calculate the statistical properties of subhalo (galaxy) major mergers at high redshift (z ...
Allgood+112 more
core +3 more sources
Numerical simulations of dwarf galaxy merger trees [PDF]
We investigate the evolution of dwarf galaxies using N -body/SPH simulations that incorporate their formation histories through merger trees constructed using the ex- tended Press-Schechter formalism.
Cloet-Osselaer, Annelies+5 more
core +3 more sources
Formation of a Spiral Galaxy in a Major Merger [PDF]
submitted to ApJL, 4 ...
Springel, Volker, Hernquist, Lars
openaire +4 more sources
ABSTRACT As the urgency to address global crises such as climate change and inequality intensifies, the concept of regenerative development has emerged as a transformative approach going beyond sustainability to actively restore and enhance both ecological and social systems.
Leonie Paul+3 more
wiley +1 more source
Mechanisms for quenching star formation in galaxies remain hotly debated, with galaxy mergers an oft-proposed pathway. In Ellison et al. (2022) we tested this scenario by quantifying the fraction of recently and rapidly quenched post-starbursts (PSBs) in
Sara Ellison+5 more
doaj +1 more source
Cosmo-Paleontology: Statistics of Fossil Groups in a Gravity-Only Simulation
We present a detailed study of fossil group candidates identified in "Last Journey", a gravity-only cosmological simulation covering a $(3.4\, h^{-1}\mathrm{Gpc})^3$ volume with a particle mass resolution of $m_p \approx 2.7 \times 10^9\, h^{-1}\mathrm{M}
Aurora Cossairt+5 more
doaj +1 more source
The Fall of a Giant. Chemical evolution of Enceladus, alias the Gaia Sausage [PDF]
We present the first chemical evolution model for Enceladus, alias the Gaia Sausage, to investigate the star formation history of one of the most massive satellites accreted by the Milky Way during a major merger event.
Aguirre, Victor Silva+6 more
core +4 more sources
Sersic properties of disc galaxy mergers [PDF]
Sersic parameters characterising the density profiles of remnants formed in collision-less disc galaxy mergers are obtained; no bulge is included in our simulations. For the luminous component we find that the Sersic index is n ~ (1.5,5.3) with ~ 3 +/- 1 and an effective radius of R_e ~ (1.6,12.9) kpc with ~ 5 +/- 3 kpc.
Hector Aceves+2 more
openaire +3 more sources
LGBTQ+ Affirmative Care Training in Counselor Education: A Community‐Based Inquiry
ABSTRACT Counselor educators, counselors‐in‐training, and LGBTQ+ community members engaged in a community‐based qualitative inquiry exploring LGBTQ+ affirmative care education. Findings revealed counselor educators’ components and delivery of content, developmental implications for applying LGBTQ+ affirmative care, and gaps between education and LGBTQ+
Nancy E. Thacker Darrow+2 more
wiley +1 more source
Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages
While supermassive black holes are ubiquitous features of galactic nuclei, only a small minority are observed during episodes of luminous accretion. The physical mechanism(s) driving the onset of fueling and ignition in these active galactic nuclei (AGN)
Peter Breiding+17 more
doaj +1 more source