591 high velocity stars in the Galactic halo selected from LAMOST DR7 and Gaia DR2
Yin-Bi Li, A-Li Luo, You-Jun Lu, Xue-Sen Zhang, Jiao Li, Rui Wang,, Fang Zuo, Maosheng Xiang, Yuan-Sen Ting, T.Marchetti, Shuo Li, You-Fen Wang,, Shuo Zhang, Kohei Hattori, Yong-Heng Zhao, Hua-Wei Zhang, and Gang Zhao

TL;DR
This study identifies 591 high velocity star candidates in the Galactic halo using LAMOST DR7 and Gaia DR2 data, revealing insights into their origins, metallicities, and potential unbound status, with implications for understanding the Milky Way's formation.
Contribution
First comprehensive catalog of high velocity stars combining LAMOST DR7 spectra and Gaia DR2 data, with analysis of their kinematics, metallicities, and origins.
Findings
At least 43 stars are unbound to the Galaxy.
Most high velocity stars are metal-poor inner halo stars.
Retrograde stars tend to have lower metallicities and higher velocities.
Abstract
In this paper, we report 591 high velocity star candidates (HiVelSCs) selected from over 10 million spectra of the data release seven (DR7) of the Large Sky Area Multi-object Fiber Spectroscopic Telescope and the second Gaia data release, with three-dimensional velocities in the Galactic rest-frame larger than 445 km/s. We show that at least 43 HiVelSCs are unbound to the Galaxy with escape probabilities larger than 50%, and this number decreases to eight if the possible parallax zero-point error is corrected. Most of these HiVelSCs are metal-poor and slightly alpha-enhanced inner halo stars. Only 14% of them have [Fe/H] > -1, which may be the metal-rich "in situ" stars in halo formed in the initial collapse of the Milky Way or metal-rich stars formed in the disk or bulge but kinematically heated. The low ratio of 14% implies that the bulk of stellar halo was formed from the accretion…
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