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Project
Objectives
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The main obejctive of our project is to study in detail the
kinematics and physical conditions of a sample of active galaxies in order
to:
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to look for a possible correlation between large-scale morphological
structures and observed kinematical deviation from the standard rotational
behaviour
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to study the nature of outflows close to the active nucleus.
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Study the relation of activity to interactions or merging
phenomena.
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and finally discuss the unification models.
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