Dark Matter Annihilations in the Large Magellanic Cloud
arXiv:astro-ph/9312011 · doi:10.1016/0920-5632(94)90234-8
Abstract
The flat rotation curve obtained for the outer star clusters of the Large Magellanic Cloud is suggestive of an LMC dark matter halo. From the composite HI and star cluster rotation curve, I estimate the parameters of an isothermal dark matter halo added to a `maximum disk.' I then examine the possibility of detecting high energy gamma-rays from non-baryonic dark matter annihilations in the central region of the Large Magellanic Cloud.
2pp, plain TeX, 0
Cited by in corpus (8)
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- Evolution of Dark Matter Halos and their Radio Emissions
- Radio emission from dark matter annihilation in the Large Magellanic Cloud
- Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios