TY  -  
T1  - Shaken and stirred : the Milky Way's dark substructures 
SN  -  /  
UR  - http://hdl.handle.net/10138/181659 
T3  -  
A1  - Sawala, Till; Pihajoki, Pauli; Johansson, Peter H.; Frenk, Carlos S.; Navarro, Julio F.; Oman, Kyle A.; White, Simon D. M. 
A2  -  
PB  -  
Y1  - 2017 
LA  - eng 
AB  - The predicted abundance and properties of the low-mass substructures embedded inside larger dark matter haloes differ sharply among alternative dark matter models. Too small to host galaxies themselves, these subhaloes may still be detected via gravitational lensing or via perturbations of the Milky Way's globular cluster streams and its stellar disc. Here, we use the APOSTLE cosmological simulations to predict the abundance and the spatial and velocity distributions of subhaloes in the range 10... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - Local Group; cosmology: theory; dark matter; DWARF SPHEROIDAL GALAXIES; GLOBULAR-CLUSTER STREAMS; COLD STELLAR STREAM; DIGITAL SKY SURVEY; MATTER HALOES; SATELLITE GALAXIES; GALACTIC DISKS; COSMOLOGICAL SIMULATIONS; OVERABUNDANCE PROBLEM; RADIAL-DISTRIBUTION; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -