Results 51 to 60 of about 30,715 (290)
Assembly of the outer Galactic stellar halo in the hierarchical model
We provide a set of numerical N-body simulations for studying the formation of the outer Milky Ways's stellar halo through accretion events. After simulating minor mergers of prograde and retrograde orbiting satellite halo with a Dark Matter main halo ...
Adelman-McCarthy +15 more
core +1 more source
A mass-dependent density profile for dark matter haloes including the influence of galaxy formation [PDF]
We introduce a mass-dependent density profile to describe the distribution of dark matter within galaxies, which takes into account the stellar-to-halo mass dependence of the response of dark matter to baryonic processes.
Aaron A. Dutton +86 more
core +2 more sources
Stellar haloes of simulated Milky-Way-like galaxies: chemical and kinematic properties [PDF]
12 pages, 6 figures. Accepted version.
P. B. Tissera +3 more
openaire +3 more sources
The Dichotomy of the Halo of the Milky Way
We summarize evidence that the halo of the Milky Way comprises two different, and broadly overlapping, stellar components. The two structures exhibit different chemical compositions, spatial distributions, and kinematics.
Akira Ohnishi +8 more
core +1 more source
The Milky Way's stellar halo - lumpy or triaxial?
10 pages, 10 figs, to appear in proceedings of conference "Physics at the end of the Galactic Cosmic Ray Spectrum", Journal of Physics: Conf. series, eds. G.
Newberg, Heidi Jo, Yanny, Brian
openaire +2 more sources
Are dSph galaxies Galactic building blocks?
Dwarf spheroidal galaxies (dSph) are frequently assumed to represent surviving examples of a vast now destroyed population of small systems in which many of the stars now forming the Milky Way were formed. Ongoing accretion and considerable sub-structure
Gilmore G., Asiri H.M.
doaj +1 more source
Group accretion in Milky Way-like stellar haloes
As galaxies form hierarchically, larger satellites can accrete alongside smaller companions in group infall events. This coordinated accretion is likely to have left signatures in the Milky Way's stellar halo that we can see today. Our goal is to characterise the possible groups of companions that accompanied larger known accretion events of our Galaxy,
Callingham, Thomas M., Helmi, Amina
openaire +3 more sources
Reliability of the Measured Velocity Anisotropy of the Milky Way Stellar Halo [PDF]
Abstract Determining the velocity distribution of halo stars is essential for estimating the mass of the Milky Way and for inferring its formation history. Since the stellar halo is a dynamically hot system, the velocity distribution of halo stars is well described by the three-dimensional velocity dispersions
Kohei Hattori +3 more
openaire +2 more sources
The Age of the Milky Way Inner Halo
The Milky Way galaxy is observed to have multiple components with distinct properties, such as the bulge, disk, and halo. Unraveling the assembly history of these populations provides a powerful test to the theory of galaxy formation and evolution, but ...
A Dotter +28 more
core +1 more source
Peptide‐based ligand antagonists block a Vibrio cholerae adhesin
The structure of a peptide‐binding domain of the Vibrio cholerae adhesin FrhA was solved by X‐ray crystallography, revealing how the inhibitory peptide AGYTD binds tightly at its Ca2+‐coordinated pocket. Structure‐guided design incorporating D‐amino acids enhanced binding affinity, providing a foundation for developing anti‐adhesion therapeutics ...
Mingyu Wang +9 more
wiley +1 more source

