Dark Matter Annihilations in the Large Magellanic Cloud

Details Dark Matter Annihilations in the Large Magellanic Cloud Dark Matter Annihilations in the Large Magellanic Cloud

1993-12-06

arxiv.org/abs/astro-ph/9312011v1

Nucl.Phys.Proc.Suppl. 35 (1994) 148-149

Astronomy and Astrophysics

Astrophysics

2pp, plain TeX, 0

Scientific paper

10.1016/0920-5632(94)90234-8

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.

Affiliated with

Also associated with

No associations

Rating

Dark Matter Annihilations in the Large Magellanic Cloud does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dark Matter Annihilations in the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark Matter Annihilations in the Large Magellanic Cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-566827