SOFIA observations provide the first experimental magnetic-dipole hyperfine constants for [13C II] and refined centroid frequency using astronomical data.
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6 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 6years
2026 6representative citing papers
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.
HONKAI identifies 193 dense cores in 16 clumps within three IRDCs, finding most have virial ratios >1 but mass-size relations below the massive star formation threshold and a steeper high-mass CMF slope.
New CO(2-1) observations of 112 clumps in outer Galactic clouds (14-23 kpc) yield velocity dispersion-size and mass-size power laws plus a declining virial parameter trend indicating most clumps are gravitationally unbound.
ALMA CO data in NGC 3351's CMZ shows a size-linewidth slope of 0.58, ordered motions stronger above 30 pc and random motions below, with free-fall times comparable to ordered crossing times across scales.
Gravity and turbulence together reproduce the observed j ~ R^{3/2} scaling in molecular cloud clumps, with magnetic fields creating filamentary structures whose apparent match may be an artifact.
citing papers explorer
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Space as a spectroscopic laboratory: High-resolution spectroscopy of the [$^{13}$C II] hyperfine structure with SOFIA/upGREAT
SOFIA observations provide the first experimental magnetic-dipole hyperfine constants for [13C II] and refined centroid frequency using astronomical data.
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ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser
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.
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A tool of Hierarchical cOre ideNtification and Kinematic property AssIgnment (HONKAI) for Dense Cores
HONKAI identifies 193 dense cores in 16 clumps within three IRDCs, finding most have virial ratios >1 but mass-size relations below the massive star formation threshold and a steeper high-mass CMF slope.
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Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations
New CO(2-1) observations of 112 clumps in outer Galactic clouds (14-23 kpc) yield velocity dispersion-size and mass-size power laws plus a declining virial parameter trend indicating most clumps are gravitationally unbound.
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Multi-scale Gas Structure and Dynamics in an Extragalactic Central Molecular Zone
ALMA CO data in NGC 3351's CMZ shows a size-linewidth slope of 0.58, ordered motions stronger above 30 pc and random motions below, with free-fall times comparable to ordered crossing times across scales.
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On the role of gravity, turbulence, and the magnetic field in angular momentum transfer within molecular clouds
Gravity and turbulence together reproduce the observed j ~ R^{3/2} scaling in molecular cloud clumps, with magnetic fields creating filamentary structures whose apparent match may be an artifact.