Results 71 to 80 of about 8,080,766 (192)

Importance of Initial Condition on Bar Secular Evolution: Role of Halo Angular Momentum Distribution Discontinuity

open access: yesThe Astrophysical Journal
The dark matter halo properties, for example, mass, spin, and concentration, play a significant role in the formation and evolution of bars in disk galaxies.
Sandeep Kumar Kataria, Juntai Shen
doaj   +1 more source

Milky Way Gas Dynamics [PDF]

open access: yes, 2018
The Milky Way is made up of a central bar, a disk with embedded spiral arms, and a dark matter halo. Observational and theoretical constraints for the characteristic parameters of these components will be presented, with emphasis on the constraints from ...
Gerhard, Ortwin, Englmaier, Peter
core  

Ursa Major III/UNIONS 1: The Darkest Galaxy Ever Discovered?

open access: yesThe Astrophysical Journal
The recently discovered stellar system Ursa Major III/UNIONS 1 (UMa3/U1) is the faintest known Milky Way satellite to date. With a stellar mass of ${16}_{-5}^{+6}\,{M}_{\odot }$ and a half-light radius of 3 ± 1 pc, it is either the darkest galaxy ever ...
Raphaël Errani   +3 more
doaj   +1 more source

Dark matter spiral arms in Milky Way-like halos

open access: yesAstronomy & Astrophysics
Context. The coupling between the dark matter (DM) halo and the stellar disc is a key factor in galactic evolution. While the interaction between structures like the Galactic bar and DM halos has been explored (e.g. slowing down of the bar due to dynamical friction), the effect of spiral arms on the DM halo distribution has received limited attention ...
Marcel Bernet   +11 more
openaire   +3 more sources

What's up in the Milky Way? The orientation of the disc relative to the triaxial halo [PDF]

open access: yes, 2013
Models of the Sagittarius stream have consistently found that the Milky Way disc is oriented such that its short axis is along the intermediate axis of the triaxial dark matter halo.
Roškar, R   +22 more
core   +1 more source

The clustering of dark matter, haloes & galaxies [PDF]

open access: yes, 2008
In this thesis I study the spatial distribution of galaxies, haloes and dark matter particles using a suite of state-of-art cosmological N-body simulations of the growth structure in the Universe.
Angulo de la Fuente, Raúl Esteban
core  

Search for dark matter candidates and large extra dimensions in events with a jet and missing transverse momentum with the ATLAS detector [PDF]

open access: yes, 2013
A search for new phenomena in events with a high-energy jet and large missing transverse momentum is performed using data from proton-proton collisions at √s=7 TeV with the ATLAS experiment at the Large Hadron Collider.
Jones, G. (Graham)   +2 more
core   +1 more source

Dark Matter Halo Tumbling Induced by Torques from Massive Mergers

open access: yesThe Astrophysical Journal
Dark matter halos exhibit slow tumbling known as “figure rotation.” Figure rotation occurs in roughly 80% of isolated ΛCDM halos and is relatively unaffected by baryonic feedback, making it an attractive and relatively unexplored test for ΛCDM.
Neil Ash, Monica Valluri
doaj   +1 more source

Simulations of satellite tidal debris in the Milky Way halo

open access: yes, 2020
Aims. We study the distribution of the stellar and dark matter debris of the Milky Way satellites. Methods. For the first time we address the question of the tidal disruption of satellites in simulations by utilising simultaneously (a) a realistic set of
Andreas Just   +3 more
core   +1 more source

Challenges in Binary Pulsar Timing Detection of Dark Matter Subhalos

open access: yesThe Astrophysical Journal Letters
Recently, binary pulsar timing has been proposed as a viable probe of dark matter subhalos with masses of ∼10 ^7 M _⊙ in the solar neighborhood.
Zheng-Long Wang   +3 more
doaj   +1 more source

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