Abstract
We investigated the formation of the Hercules stream in the model Galactic disk that includes the outer elliptical rings \(R_{1}\) and \(R_{2}\) located near the Outer Lindblad Resonance (OLR) of the bar. Most stars in the Hercules region have orbits elongated perpendicular to the bar and support the outer ring \(R_{1}\) while those in the anti-Hercules region have orbits elongated parallel to the bar and support the \(R_{2}\) ring. Stars of the Gaia DR3 catalog located in the Hercules region are more strongly concentrated toward the Galactic plane than stars of the anti-Hercules region, which prevents comparison between their physical characteristics, since selection effects affect these samples differently.
