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The Milky Way is surrounded by dozens of dwarf galaxies thought to be relics of the first galaxies in the universe. Among the most primitive of these galactic fossils is Tucana II -- an ultrafaint dwa...
Observations of two galaxies made with the National Science Foundation-funded Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope suggest that large galaxies formed faster than scienti...
Reconciling dwarf galaxies with dark matter     dwarf galaxies  dark matter       font style='font-size:12px;'> 2016/9/12
Dwarf galaxies are enigmas wrapped in riddles. Although they are the smallest galaxies, they represent some of the biggest mysteries about our universe. While many dwarf galaxies surround our own Milk...
High-redshift galaxies in cold dark matter models     dark matter  large-scale structure of the Universe       font style='font-size:12px;'> 2014/12/26
We use hydrodynamic cosmological simulations to predict the star formation properties of high-redshift galaxies (z = 2-6) in five variants of the inflationary cold dark matter scenario, paying particu...
Using a hydrodynamic simulation of a cold dark matter universe with a cosmological constant, we investigate the "X-ray forest" absorption imprinted on the spectra of background quasars by the interven...
Dark Matter Constraints from the Sagittarius Dwarf and Tail System     the Sagittarius Dwarf  Tail System       font style='font-size:12px;'> 2014/12/24
2MASS has provided a three-dimensional map of the >360 degree, wrapped tidal tails of the Sagittarius (Sgr) dwarf spheroidal galaxy, as traced by M giant stars. With the inclusion of radial velocity d...
Bar-induced evolution of dark matter cusps     kinematics and dynamics  structure       font style='font-size:12px;'> 2014/12/24
The evolution of a stellar bar transforms not only the galactic disc, but also the host dark matter halo. We present high-resolution, fully self-consistent N-body simulations that clearly demonstrate ...
N-body simulations predict that cold dark matter (CDM) halo-assembly occurs in two phases: (i) a fast-accretion phase with a rapidly deepening potential well; and (ii) a slow-accretion phase character...
Dark matter halo response to the disc growth     dark matter  evolution  halos       font style='font-size:12px;'> 2014/12/23
We consider the sensitivity of the circular-orbit adiabatic contraction approximation to the baryon condensation rate and the orbital structure of dark matter haloes in the Λ cold dark matter (ΛCDM) p...
Baryon dynamics, dark matter substructure, and galaxies     formation  large-scale structure of universe       font style='font-size:12px;'> 2014/12/23
By comparing a collisionless cosmological N-body simulation (DM) to a smoothed particle hydrodynamics simulation (SPH) with the same initial conditions, we investigate the correspondence between dark ...
The dynamics of satellite disruption in cold dark matter haloes     numerical  N-body simulation       font style='font-size:12px;'> 2014/12/22
We investigate the physical mechanisms of tidal heating and satellite disruption in cold dark matter host haloes using N-body simulations based on cosmological initial conditions. We show the importan...
Dark Matter Halos: Assembly, Clustering and Sub-halo Accretion     Dark matter  Galaxy formation  Halos       font style='font-size:12px;'> 2014/12/9
I carried out systematic studies on the assembly history of dark matter halos, using numerical simulations and semi-analytical methods. First, I look into dark halo mass assembly history. I confirmed ...
Like a bullet wrapped in a full metal jacket, a high-velocity hydrogen cloud hurtling toward the Milky Way appears to be encased in a shell of dark matter, according to a new analysis of data from the...
According to the polar effect in the hyperspherical universe, we realize thatDark matter may be invisible gravitational ghost images originating from the matter around the poles and not the real na...
Modern cosmology suggests that the Universe contains two dark components -- dark matter and dark energy -- both unkown in laboratory physics and both lacking direct evidence. Alternatively, a unified ...

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