Abstract
The Saint-Malo massif provides an example of a gneiss dome with a migmatitic core. The results of a structural analysis are used to describe a structural zonation around the migmatitic core, and a dynamic model of the massif is proposed. A comparison of these results with experimental models of gneiss domes shows that this zonation is the product of diapirism.
Publisher
Canadian Science Publishing
Subject
General Earth and Planetary Sciences
Cited by
26 articles.
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