Results 141 to 150 of about 12,786 (266)
Self-interacting Dark Matter Interpretation of Crater II
The satellite galaxy Crater II of the Milky Way is extremely cold and exceptionally diffuse. These unusual properties are challenging to understand in the standard model of cold dark matter.
Xingyu Zhang +3 more
doaj +1 more source
The Origin of High-velocity Stars Considering the Impact of the Large Magellanic Cloud
Utilizing astrometric parameters sourced from Gaia Data Release 3 and radial velocities obtained from various spectroscopic surveys, we identify 519 high-velocity stars (HiVels) with a total velocity in the Galactocentric rest frame greater than 70% of ...
Jiwei Liao +7 more
doaj +1 more source
In this paper, we explore the Oscillating Asymmetric Dark Matter (OADM) model to address the core-cusp problem, aiming to resolve the discrepancy between the predictions of the $$\Lambda \textrm{CDM}$$ Λ CDM cosmological model and the observed dark ...
Júlia G. Mamprim +4 more
doaj +1 more source
Assessing the Association between the Globular Cluster NGC 4147 and the Sagittarius Dwarf Galaxy
The potential association of the globular cluster (GC) NGC 4147 with the Sagittarius (Sgr) dwarf spheroidal galaxy has been proposed due to their comparable locations and radial velocities. However, there are still debates about this connection.
Ying-Hua Zhang +3 more
doaj +1 more source
The dynamical and chemical evolution of dwarf spheroidal galaxies with GEAR [PDF]
Yves Revaz, P. Jablonka
openalex +1 more source
Chemical feature of Eu abundance in the Draco dwarf spheroidal galaxy [PDF]
Takuji Tsujimoto +3 more
openalex +1 more source
Sommerfeld-enhanced dark matter searches with dwarf spheroidal galaxies [PDF]
Shin’ichiro Ando, Koji Ishiwata
openalex +1 more source
WFPC2 Observations of the Carina Dwarf Spheroidal Galaxy.
We present our analysis of Hubble Space Telescope Wide Field Planetary Camera 2 observations in F555W (~V) and F814W (~I) of the Carina dwarf spheroidal galaxy. The resulting V vs (V-I) color-magnitude diagrams reach V ~ 27.1 mag. The reddening of Carina is estimated to be E(V-I) = 0.08 +- 0.02 mag.
openaire +2 more sources
The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data
We investigate the spatial distribution, kinematics, and metallicity of stars in the Draco dwarf spheroidal galaxy using data from the Dark Energy Spectroscopic Instrument (DESI).
J. Ding +42 more
doaj +1 more source
Variable stars in Fornax dwarf spheroidal galaxy
10 pages, 9 figures, to appear in the Proceedings of "Resolved Stellar Populations", 2005, Cancun ...
Greco, C. +12 more
openaire +2 more sources

