Univ. Politecnica de Catalunya

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Papers (1)

1. Why are Halo Density Profiles Stable at Formation? astro-ph · 1998 · author #4

Mentions

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Frequent Coauthors

• (2) Dep. Astronomia i Meteorologia 1 shared papers
• A. Raig 1 shared papers
• E. Salvador-Sole (2) ((1) Dep. Matematica Aplicada II 1 shared papers
• G. Gonzalez-Casado (1) 1 shared papers
• Univ. Barcelona) 1 shared papers