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A Collimated Protostellar Outflow Likely Driven by Jet and Reshaped by Environment in the Sagittarius C Cloud of the Central Molecular Zone
The Central Molecular Zone (CMZ) at the center of the Galaxy provides a nearby laboratory for studying star formation under extreme physical and chemical conditions. Recent ALMA (Atacama Large Millimeter/Submillimeter Array) observations have identified 43 candidate protostellar outflows in three CM
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