High resolution simulations of the Local Group in the CLUES project

Details High resolution simulations of the Local Group in the CLUES project High resolution simulations of the Local Group in the CLUES project

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011hsa6.conf..259m&link_type=abstract

Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society (SEA), held

Astronomy and Astrophysics

Astrophysics

Scientific paper

Constrained simulations with different resolution, cosmological models and dark matter components were carried out within the CLUES project. They allowed us to study some important properties for both the Local Group (LG) and its environment. We have studied the evolution and structure of the main galactic haloes in the Local Group and their galaxies as well as the substructures in these haloes. We paid special attention to the missing satellite problem in the standard Cold Dark Matter scenario and studied whether the possible biases between dark and luminous components could alleviate or even solve this problem.

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