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Pattern speeds in the Milky Way

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

A brief review is given of different methods used to determine the pattern speeds of the Galactic bar and spiral arms. The Galactic bar rotates rapidly, with corotation about halfway between the Galactic center and the Sun, and outer Lindblad resonance not far from the solar orbit, R0. The Galactic spiral arms currently rotate with a distinctly slower pattern speed, such that corotation is just outside R0. Both structures therefore seem dynamically decoupled.

fields

astro-ph.GA 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Start of orbit librations and the bar growth timescale

astro-ph.GA · 2026-06-25 · unverdicted · novelty 6.0

Dynamical models with varying bar growth times Tg show that librations start at 54% of maximum bar strength (Qb=0.170) via proportional shifts in VR profiles.

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Showing 1 of 1 citing paper.

  • Start of orbit librations and the bar growth timescale astro-ph.GA · 2026-06-25 · unverdicted · none · ref 40 · internal anchor

    Dynamical models with varying bar growth times Tg show that librations start at 54% of maximum bar strength (Qb=0.170) via proportional shifts in VR profiles.