Tree-ring structure of Galactic bar resonance
Rimpei Chiba, Ralph Sch\"onrich

TL;DR
This paper uses the structure of star metallicity in the galactic resonance to measure the Milky Way's bar pattern speed, confirming its slow deceleration and supporting dark matter presence.
Contribution
It introduces a novel method to measure the galactic bar's pattern speed using star metallicity gradients and resonance trapping, providing new insights into galactic dynamics.
Findings
Measured the bar's pattern speed as 35.5 km/s/kpc.
Confirmed the bar has decelerated by over 24%.
Supported the existence of a dark matter halo.
Abstract
Galaxy models have long predicted that galactic bars slow down by losing angular momentum to their postulated dark haloes. When the bar slows down, resonance sweeps radially outwards through the galactic disc while growing in volume, thereby sequentially capturing new stars at its surface/separatrix. Since trapped stars conserve their action of libration, which measures the relative distance to the resonance centre, the order of capturing is preserved: the surface of the resonance is dominated by stars captured recently at large radius, while the core of the resonance is occupied by stars trapped early at small radius. The slow-down of the bar thus results in a rising mean metallicity of trapped stars from the surface towards the centre of the resonance as the Galaxy's metallicity declines towards large radii. This argument, when applied to Solar neighbourhood stars, allows a novel…
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