The James Webb Space Telescope prompts a rethink of how galaxies form. [PDF]
Mann A.
europepmc +1 more source
DIFFERENT APPROACHES FOR DARK MATTER HALOS OF CLUSTERS OF GALAXIES
Ruslan Brilenkov +2 more
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Dynamical Imprint of Dark Matter Halo and Interstellar Gas on Spiral Structure in Disk Galaxies [PDF]
Soumavo Ghosh
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Dark matter halos and scaling relations of extremely massive spiral galaxies from extended H
Enrico M. Di Teodoro +8 more
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The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles [PDF]
Jeremy J. Webb, Enrico Vesperini
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Relation between the Local Width and Linear Halo Mass Density of Cosmic Filaments
Large-scale cosmic filaments may have played an important role in shaping the properties of galaxies. Meanwhile, cosmic filaments are believed to harbor a substantial portion of the missing baryons at redshift z < 2.
Weishan Zhu +4 more
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Globular cluster ejection, infall, and the host dark matter halo of the Pegasus dwarf galaxy
Ryan Leaman +12 more
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The Tidal Torque Theory Revisited. I. Protohalo Angular Momentum
In tidal torque theory, the angular momentum (AM) of dark matter halos arises from the tidal torque suffered by aspherical collapsing patches due to surrounding mass fluctuations.
Eduard Salvador-Solé, Alberto Manrique
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Halo Bias in the Peak Model: A First-principles Nonparametric Approach
The Press–Schechter (PS) and excursion set (ES) models of structure formation fail in reproducing the halo bias found in simulations, while the ES-peaks' formalism built in the peak model reproduces it only at high masses and does not address in a fully ...
Eduard Salvador-Solé, Alberto Manrique
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