Galactic disks precess ubiquitously from tidal torques, causing warps, orbital heating, and radial alignments of satellites.
Connection to morphology, halo spin, and black hole mass
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
TNG50 shows most massive high-z star-forming galaxies are dynamically hotter than ALMA data indicate, with rare cold discs forming from aligned accretion and evolving into one-third discs and two-thirds early-type galaxies by z=0.
citing papers explorer
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A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications
Galactic disks precess ubiquitously from tidal torques, causing warps, orbital heating, and radial alignments of satellites.
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Dynamically cold discs in high-redshift galaxies: comparison between ALMA observations and TNG50
TNG50 shows most massive high-z star-forming galaxies are dynamically hotter than ALMA data indicate, with rare cold discs forming from aligned accretion and evolving into one-third discs and two-thirds early-type galaxies by z=0.