Tides in clouds: control of star formation by long-range gravitational force
Guang-Xing Li

TL;DR
This study reveals that long-range gravitational tides in molecular clouds regulate star formation by controlling gas fragmentation and transport, explaining the hierarchical clustering observed in star-forming regions.
Contribution
It introduces a novel analysis of tidal forces in cloud evolution, highlighting their dominant role in shaping star formation patterns, based on 3D density and gravitational potential modeling.
Findings
Fragmentation occurs mainly in isolated high-density regions.
Most of the gas is under extensive tides that suppress fragmentation.
Tidal forces explain the hierarchical and localized star formation pattern.
Abstract
Gravity drives the collapse of molecular clouds through which stars form, yet the exact role of gravity in cloud collapse remains a complex issue. Studies point to a picture where star formation occurs in clusters. In a typical, pc-sized cluster-forming region, the collapse is hierarchical, and the stars should be born from regions of even smaller sizes (). The origin of this spatial arrangement remains under investigation. Based on a high-quality surface density map towards the Perseus region, we construct a 3D density structure, compute the gravitational potential, and derive eigenvalues of the tidal tensor (, , , ), analyze the behavior of gravity at every location and reveal its multiple roles in cloud evolution. We find that fragmentation is…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Scientific Research and Discoveries
