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Characterizing the high-velocity stars of RAVE: the discovery of a metal-rich halo star born in the Galactic disc

Hawkins, K.; Kordopatis, G.; Gilmore, G.; Masseron, T.; Wyse, R. F. G.; Ruchti, G.; Bienaymé, O.; Bland-Hawthorn, J.; Boeche, C.; Freeman, K.; Gibson, B. K.; Grebel, E. K.; Helmi, A.; Kunder, A.; Munari, U.; Navarro, J. F.; Parker, Q. A.; Reid, W. A.; Scholz, R. D.; Seabroke, G.; Siebert, A.; Steinmetz, M.; Watson, F.; Zwitter, T.

Authors

K. Hawkins

G. Kordopatis

G. Gilmore

T. Masseron

R. F. G. Wyse

G. Ruchti

O. Bienaymé

J. Bland-Hawthorn

C. Boeche

K. Freeman

B. K. Gibson

E. K. Grebel

A. Helmi

A. Kunder

U. Munari

J. F. Navarro

Q. A. Parker

W. A. Reid

R. D. Scholz

G. Seabroke

A. Siebert

M. Steinmetz

F. Watson

T. Zwitter



Abstract

© 2015 The Authors. We aim to characterize high-velocity (HiVel) stars in the solar vicinity both chemically and kinematically using the fourth data release of the RAdial Velocity Experiment (RAVE). We used a sample of 57HiVel starswith Galactic rest-frame velocities larger than 275 km s-1.With 6D position and velocity information, we integrated the orbits of the HiVel stars and found that, on average, they reach out to 13 kpc from the Galactic plane and have relatively eccentric orbits consistent with the Galactic halo. Using the stellar parameters and [α/Fe] estimates from RAVE, we found the metallicity distribution of the HiVel stars peak at [M/H] = -1.2 dex and is chemically consistent with the inner halo. There are a few notable exceptions that include a hypervelocity star candidate, an extremely HiVel bound halo star, and one star that is kinematically consistent with the halo but chemically consistent with the disc. High-resolution spectra were obtained for the metal-rich HiVel star candidate and the second highest velocity star in the sample. Using these high-resolution data, we report the discovery of a metal-rich halo star that has likely been dynamically ejected into the halo from the Galactic thick disc. This discovery could aid in explaining the assembly of the most metal-rich component of the Galactic halo.

Citation

Hawkins, K., Kordopatis, G., Gilmore, G., Masseron, T., Wyse, R. F. G., Ruchti, G., Bienaymé, O., Bland-Hawthorn, J., Boeche, C., Freeman, K., Gibson, B. K., Grebel, E. K., Helmi, A., Kunder, A., Munari, U., Navarro, J. F., Parker, Q. A., Reid, W. A., Scholz, R. D., Seabroke, G., …Zwitter, T. (2015). Characterizing the high-velocity stars of RAVE: the discovery of a metal-rich halo star born in the Galactic disc. Monthly notices of the Royal Astronomical Society, 447(2), 2046-2058. https://doi.org/10.1093/mnras/stu2574

Journal Article Type Article
Acceptance Date Dec 2, 2014
Online Publication Date Jan 3, 2015
Publication Date Feb 21, 2015
Deposit Date Jun 29, 2018
Publicly Available Date Jul 11, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 447
Issue 2
Pages 2046-2058
DOI https://doi.org/10.1093/mnras/stu2574
Keywords Galaxy : abundances; Galaxy : halo; Galaxy : kinematics and dynamics
Public URL https://hull-repository.worktribe.com/output/543728
Publisher URL https://academic.oup.com/mnras/article/447/2/2046/2593778
Contract Date Jun 29, 2018

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