A Galactic Ring of Minimum Stellar Density Near the Solar Orbit Radius
Douglas A. Barros, Jacques R. D. L\'epine, Thiago C. Junqueira

TL;DR
This paper investigates how long-lived spiral structures in the Galaxy create a minimum stellar density near the corotation radius, affecting stellar migration and the Galaxy's mass distribution.
Contribution
It demonstrates the formation of a stellar density minimum at corotation due to secular angular momentum transfer, supported by simulations and observational evidence.
Findings
A minimum stellar density of 30-40% of background at corotation.
Secular angular momentum transfer enables radial migration across corotation.
The solar orbit is within a stellar density minimum, affecting Galactic mass estimates.
Abstract
We analyse the secular effects of a long-lived Galactic spiral structure on the stellar orbits with mean radii close to the corotation resonance. By test-particle simulations and different spiral potential models with parameters constrained on observations, we verified the formation of a minimum with amplitude ~ 30% - 40% of the background disk stellar density at corotation. Such minimum is formed by the secular angular momentum transfer between stars and the spiral density wave on both sides of corotation. We demonstrate that the secular loss (gain) of angular momentum and decrease (increase) of mean orbital radius of stars just inside (outside) corotation can counterbalance the opposite trend of exchange of angular momentum shown by stars orbiting the librational points L_4/5 at the corotation circle. Such secular processes actually allow steady spiral waves to promote radial…
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