Filaments in Warm Dark Matter

Details Filaments in Warm Dark Matter Filaments in Warm Dark Matter

2002-06-20

arxiv.org/abs/astro-ph/0206346v1

Astronomy and Astrophysics

Astrophysics

1 page, 1 figure, rmaa.cls, to appear in 'Galaxy evolution: theory and observations', Eds. V. Avila-Reese, C. Firmani, C. Fren

Scientific paper

Using Warm Dark Matter rather then Cold Dark Matter we are able to solve the over-production of satellite galaxies orbiting in galactic haloes. Moreover, we can show that this model leads to interesting new results in terms of the history and large-scale distribution of low-mass objects as well as the formation of filamentary structures when being compared to the standard CDM scenario.

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