Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
Statistically significant gamma-ray detection from young stellar objects indicates hadronic particle acceleration in protostellar jets with output scaling to bolometric luminosity.
citing papers explorer
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Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow
Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.
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Evidence for protostellar jets as a population of hadronic gamma-ray sources
Statistically significant gamma-ray detection from young stellar objects indicates hadronic particle acceleration in protostellar jets with output scaling to bolometric luminosity.