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arXiv · 1702.06541

Revisiting the Tale of Hercules: how stars orbiting the Lagrange points visit the Sun

Angeles Pérez-Villegas·Matthieu Portail·Christopher Wegg·Ortwin Gerhard
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Abstract

We propose a novel explanation for the Hercules stream consistent with recent measurements of the extent and pattern speed of the Galactic bar. We have adapted a made-to-measure dynamical model tailored for the Milky Way to investigate the kinematics of the solar neighborhood (SNd). The model matches the 3D density of the red clump giant stars (RCGs) in the bulge and bar as well as stellar kinematics in the inner Galaxy, with a pattern speed of 39 km s$^{-1}$ kpc$^{-1}$. Cross-matching this model with the $Gaia$ DR1 TGAS data combined with RAVE and LAMOST radial velocities, we find that the model naturally predicts a bimodality in the $U\!-\!V$-velocity distribution for nearby stars which is in good agreement with the Hercules stream. In the model, the Hercules stream is made of stars orbiting the Lagrange points of the bar which move outward from the bar's corotation radius to visit the SNd. While the model is not yet a quantitative fit of the velocity distribution, the new picture naturally predicts that the Hercules stream is more prominent inward from the Sun and nearly absent only a few $100$ pc outward of the Sun, and plausibly explains that Hercules is prominent in old and metal-rich stars.

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Angeles Pérez-Villegas, Matthieu Portail, Christopher Wegg, Ortwin Gerhard. 2017-02-21. Revisiting the Tale of Hercules: how stars orbiting the Lagrange points visit the Sun. https://doi.org/10.3847/2041-8213/aa6c26

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