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Molecular material in the Bubble of the Galactic Center

Abstract The Galactic Center (GC) is one of the more extreme environments in the Galaxy. The so call Bubble of the GC presents structures that do not match with the general behavior of the inner Central Molecular Zone (CMZ). In this work we study the molecular emission related to the observable ionized gas emitted by this Bubble. We find dense pockets of gas and bubble like structures in the velocity domain.