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Unveiling a Network of Parallel Filaments in the Infrared Dark Cloud G14.225–0.506
UploadEarly Stages of Cluster Formation: Fragmentation of Massive Dense Cores Down to ≲ 1000 Au
UploadIntermediate-Mass Hot Cores at ∼500 Au: Disks or Outflows?
UploadDense gas and the nature of the outflows
UploadN2H+depletion in the massive protostellar cluster AFGL 5142
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