Confronting HST Observations of Dwarf Spheroidals with Theory

Details Confronting HST Observations of Dwarf Spheroidals with Theory Confronting HST Observations of Dwarf Spheroidals with Theory

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10283g&link_type=abstract

HST Proposal ID #10283

Mathematics

Logic

Hst Proposal Id #10283 Cosmology

Scientific paper

We will continue our work on using advanced cosmological simulations to model the formation and evolution of dwarfs spheroidal galaxies. Our previous simulations were able to fully resolve the internal structure of dwarf spheroidals formed before the reionization epoch. In this cycle we will incorporate results from our previous simulations into a large-scale N-body only code to model the formation of the Local Group and to relate the results of our gas-dynamical simulations to the present distribution of dwarf spheroidals in the Local Group. The results of our simulations will be compared to the observational data, including the color-magnitude diagrams of dwarfs spheroidals, obtained by the HST.

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