Hostname: page-component-6b989bf9dc-llglr Total loading time: 0 Render date: 2024-04-14T17:36:48.037Z Has data issue: false hasContentIssue false
  • English
  • Français

Dwarf galaxies are among the best places to probe the nature of dark matter

Published online by Cambridge University Press:  08 November 2005

S. Colafrancesco
S. Colafrancesco
Affiliation:
INAF - Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio, I00040, Italy. email: cola@mporzio.astro.it
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I discuss here the main physical constraints on Dark Matter particles that can be obtained by the study of the astrophysical signals produced by their annihilation within Dwarf Galaxies. The present results are obtained in the framework of neutralino Dark Matter scenarios and under the assumption that Dwarf Galaxies are dominated by Dark Matter.

Keywords

Dwarf galaxiesDark MatterCosmology
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Colloquium C198: Near-Field Cosmology with Dwarf Elliptical Galaxies , March 2005 , pp. 229 - 234
Copyright
© 2005 International Astronomical Union