On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation

Cosmological hydrodynamical simulations are studied in order to analyse generic trends for the stellar, baryonic and halo mass assembly of low-mass galaxies (M* < 3 × 1010M⊙) as a function of their present halo mass, in the context of the λcold dark matter (λCDM) scenario and common subgrid p...

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Autores principales: De Rossi, M.E., Avila-Reese, V., Tissera, P.B., González-Samaniego, A., Pedrosa, S.E.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v435_n3_p2736_DeRossi
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