Signatures of Dark Matter Burning in Nuclear Star Clusters
In order to characterize how dark matter (DM) annihilation inside stars changes the aspect of a stellar cluster, we computed the evolution until the ignition of the He burning of stars from 0.7 M sun to 3.5 M sun within halos of DM with different characteristics. We found that, when a cluster is sur...
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| Format: | article |
| Language: | eng |
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2012
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| Online Access: | http://hdl.handle.net/10174/3886 |
| Country: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/3886 |