Evolution of Low Mass Galactic Subhalos and Dependence on Concentration

Abstract

We carry out a detailed study of the orbital dynamics and structural evolution of over 6000 subhalos in the Via Lactea II simulation, from infall to present. By analyzing subhalos with masses down to m = 4e5 Msun, we find that lower mass subhalos, which are not strongly affected by dynamical friction, exhibit behaviors qualitatively different from those found previously for more massive ones. Furthermore, there is a clear trend of subhalos that fell into the host earlier being less concentrated. We show that the concentration at infall characterizes various aspects of subhalo evolution. In particular, tidal effects truncate the growth of less concentrated subhalos at larger distances from the host; subhalos with smaller concentrations have larger infall radii. The concentration at infall is further shown to be a determining factor for the subsequent mass loss of subhalos within the host, and also for the evolution of their internal structure in the v_max-r_max plane. Our findings raise the prospects of using the concentration to predict the tidal evolution of subhalos, which will be useful for obtaining analytic models of galaxy formation, as well as for near field cosmology.

Accepted for publication in the Astrophysical Journal

References in corpus (10)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• The Tidal Evolution of Local Group Dwarf Spheroidals
• A fitting formula for the merger timescale of galaxies in hierarchical clustering
• The Population of Dark Matter Subhaloes: Mass Functions and Average Mass Loss Rates
• The Unorthodox Orbits of Substructure Halos
• Cosmic Ménage à Trois: The Origin of Satellite Galaxies On Extreme Orbits
• Early supersymmetric cold dark matter substructure
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• The Graininess of Dark Matter Haloes
• Nonlinear evolution of dark matter subhalos and applications to warm dark matter

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