Results 1 to 10 of about 617 (181)

The Structure of Dark Matter Halos in Dwarf Galaxies [PDF]

open access: yesThe Astrophysical Journal, 1995
Some dwarf galaxies have HI rotation curves that are completely dominated by a surrounding dark matter (DM) halo (e.g. Carignan & Freeman 1988). These objects represent ideal candidates for an investigation of the density structure of low-mass DM halos as the uncertainties resulting from the subtraction of the visible component are small, even in ...
openaire   +4 more sources

Dark matter halo properties from galaxy–galaxy lensing★ [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We present results for a galaxy-galaxy lensing study based on imaging data from the Canada-France-Hawaii Telescope Legacy Survey Wide. From a 12 million object multi-colour catalogue for 124 deg^2 of photometric data in the u*g'r'i'z' filters we compute photometric redshifts (with a scatter of σ_{Δz/(1+z)} = 0.033 and an outlier rate of η=2.0 per cent ...
Brimioulle, F.   +4 more
openaire   +3 more sources

Ultra Light Axionic Dark Matter: Galactic Halos and Implications for Observations with Pulsar Timing Arrays

open access: yesGalaxies, 2018
The cold dark matter (CDM) paradigm successfully explains the cosmic structure over an enormous span of redshifts. However, it fails when probing the innermost regions of dark matter halos and the properties of the Milky Way’s dwarf galaxy satellites ...
Ivan de Martino   +5 more
doaj   +1 more source

Flat Galaxies with Dark Matter Halos—Existence and Stability [PDF]

open access: yesCommunications in Mathematical Physics, 2009
We consider a model for a flat, disk-like galaxy surrounded by a halo of dark matter, namely a Vlasov-Poisson type system with two particle species, the stars which are restricted to the galactic plane and the dark matter particles. These constituents interact only through the gravitational potential which stars and dark matter create collectively ...
Fiřt, Roman   +2 more
openaire   +2 more sources

The rise and fall of galaxy activity in dark matter haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
We use a SDSS galaxy group catalogue to study the dependence of galaxy activity on stellar mass, halo mass, and group hierarchy (centrals vs. satellites). We split our galaxy sample in star-forming galaxies, galaxies with optical AGN activity and radio sources.
Pasquali, A   +4 more
openaire   +3 more sources

Galaxy Rotation Curves and Universal Scaling Relations: Comparison between Phenomenological and Fermionic Dark Matter Profiles

open access: yesThe Astrophysical Journal, 2023
Galaxies show different halo scaling relations such as the radial acceleration relation, the mass discrepancy acceleration relation (MDAR), or the dark matter (DM) surface density relation.
A. Krut   +4 more
doaj   +1 more source

Ellipticity of dark matter haloes with galaxy-galaxy weak lensing [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
20 pages, 8 figures, matches MNRAS accepted version (includes updated discussion of systematics, no changes to conclusions)
Mandelbaum, Rachel   +4 more
openaire   +2 more sources

A Tilt in the Dark Matter Halo of the Galaxy

open access: yesThe Astrophysical Journal, 2022
Abstract Recent observations of the stellar halo have uncovered the debris of an ancient merger, Gaia–Sausage–Enceladus (GSE), estimated to have occurred ≳8 Gyr ago. Follow-up studies have associated GSE with a large-scale tilt in the stellar halo that links two well-known stellar overdensities in diagonally opposing octants of the ...
Jiwon Jesse Han   +11 more
openaire   +2 more sources

Constraining the substructure of dark matter haloes with galaxy–galaxy lensing [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
19 pages, 14 figures, accepted by ...
Li, Ran   +4 more
openaire   +2 more sources

Cosmic Reionization on Computers: Baryonic Effects on Halo Concentrations during the Epoch of Reionization

open access: yesThe Astrophysical Journal, 2023
Baryons both increase halo concentration through adiabatic contraction and expel mass through feedback processes. However, it is not well understood how the radiation fields prevalent during the epoch of reionization affect the evolution of concentration
Hanjue Zhu, Nickolay Y. Gnedin
doaj   +1 more source

Home - About - Disclaimer - Privacy