High-resolution ALMA data identify new episodic multipolar outflow lobes in W49N showing knot chains and precession wiggles, confirming high energy and indicating conserved outflow mechanisms across stellar mass ranges.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Magnetically-driven protostellar jets transport sufficient angular momentum outward to prevent massive protostars from reaching critical rotation speeds, with jet strength linked to initial formation conditions producing a variety of final stellar rotation rates.
VLA imaging and modeling of five HC HII candidates indicate most are small UC HII regions, with G40.28-0.22 as the strongest remaining HC case.
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Physical characterization and modeling of candidate Hyper-Compact HII Regions
VLA imaging and modeling of five HC HII candidates indicate most are small UC HII regions, with G40.28-0.22 as the strongest remaining HC case.