<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>

COPY SCRIPT

For further information contact us at helpdesk@openaire.eu

Filaments in Warm Dark Matter

Name: Filaments in Warm Dark Matter
Creator: Knebe, Alexander
Keywords: Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 2002Embargo end date: 01 Jan 2002Publisher:arXiv

Authors: Knebe, Alexander;

doi: 10.48550/arxiv.astro-ph/0206346

arXiv: http://arxiv.org/abs/astro-ph/0206346

Filaments in Warm Dark Matter

- Summary
- Subjects
- Metrics

Abstract

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.

1 page, 1 figure, rmaa.cls, to appear in 'Galaxy evolution: theory and observations', Eds. V. Avila-Reese, C. Firmani, C. Frenk, & C. Allen, RevMexAA SC (2002)

Related Organizations

Swinburne University of Technology
Australia

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	0
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average

Found an issue? Give us feedback

Average

Green

Related to Research communities

NEANIAS Space Research Community