Neutralino annihilation gamma-rays from clumps and the LMC
arXiv:astro-ph/0306561 · doi:10.1016/j.newar.2003.12.005
Abstract
We discuss the detectability of dark matter clumps in the Milky Way halo due to neutralino annihilation. We then focus on a known ``clump'', the Large Magellanic Cloud.
4 pages, 4 figures; to appear in New Astronomy Reviews, Proceedings of 2nd VERITAS symposium
References in corpus (3)
Cited by in corpus (5)
- Galactic Substructure and Dark Matter Annihilation in the Milky Way Halo
- Galactic Substructure and Direct Detection of Dark Matter
- The Gamma-Ray-Flux Probability Distribution Function from Galactic Halo Substructure
- Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
- Could the Fermi-LAT detect gamma-rays from dark matter annihilation in the dwarf galaxies of the Local Group?