tipa -- 10/14/2010

Bound and unbound substructures in Galaxy-scale Dark Matter haloes

Gas accretion as the origin of chemical abundance gradients in distant galaxies

The Origin of Dark Matter Halo Profiles

When A Standard Candle Flickers

Caltech Core-Collapse Project (CCCP) observations of type IIn supernovae: typical properties and implications for their progenitor stars

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