Blue-asymmetric spectral lines appear in 50-60% of dense cores within massive dark clumps, showing that gravitational collapse operates at core scales from prestellar stages onward and supports hierarchical star formation.
Shu-Ichiro Inutsuka and Shoken M
2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
Velocity gradients in sub-parsec supercritical filaments show random orientations uncorrelated with skeletons or gravity, indicating turbulence-dominated chaotic motions at small scales.
citing papers explorer
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Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps
Blue-asymmetric spectral lines appear in 50-60% of dense cores within massive dark clumps, showing that gravitational collapse operates at core scales from prestellar stages onward and supports hierarchical star formation.
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Random gas motions inside sub-parsec scale supercritical filaments
Velocity gradients in sub-parsec supercritical filaments show random orientations uncorrelated with skeletons or gravity, indicating turbulence-dominated chaotic motions at small scales.