A detailed view of filaments and sheets of the warm-hot intergalactic medium
In the context of cosmological structure formation sheets, filaments and eventually halos form due to gravitational instabilities. It is noteworthy, that at all times, the majority of the baryons in the universe does not reside in the dense halos but in the filaments and the sheets of the intergalac...
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| Format: | Doctoral Thesis |
| Language: | English |
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Universität Potsdam
2012
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| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-58038 http://opus.kobv.de/ubp/volltexte/2012/5803/ |