Jennifer Wojno
Chemical separation of disc components using RAVE
Wojno, Jennifer; Kordopatis, Georges; Steinmetz, Matthias; McMillan, Paul; Matijevič, Gal; Binney, James; Wyse, Rosemary F. G.; Boeche, Corrado; Just, Andreas; Grebel, Eva K.; Siebert, Arnaud; Bienaymé, Olivier; Gibson, Brad K.; Zwitter, Tomaž; Bland-Hawthorn, Joss; Navarro, Julio F.; Parker, Quentin A.; Reid, Warren; Seabroke, George; Watson, Fred
Authors
Georges Kordopatis
Matthias Steinmetz
Paul McMillan
Gal Matijevič
James Binney
Rosemary F. G. Wyse
Corrado Boeche
Andreas Just
Eva K. Grebel
Arnaud Siebert
Olivier Bienaymé
Brad K. Gibson
Tomaž Zwitter
Joss Bland-Hawthorn
Julio F. Navarro
Quentin A. Parker
Warren Reid
George Seabroke
Fred Watson
Abstract
© 2016 The Authors. We present evidence from the RAdial Velocity Experiment (RAVE) survey of chemically separated, kinematically distinct disc components in the solar neighbourhood.We apply probabilistic chemical selection criteria to separate our sample into a-low ('thin disc') and a-high ('thick disc') sequences. Using newly derived distances,which will be utilized in the upcoming RAVE DR5, we explore the kinematic trends as a function of metallicity for each of the disc components. For our a-low disc, we find a negative trend in the mean rotational velocity (Vf) as a function of iron abundance ([Fe/H]). We measure a positive gradient ∂Vφ/∂[Fe/H] for the a-high disc, consistent with results from high-resolution surveys.We also find differences between the a-low and a-high discs in all three components of velocity dispersion.We discuss the implications of an a-low, metal-rich population originating from the inner Galaxy, where the orbits of these stars have been significantly altered by radial mixing mechanisms in order to bring them into the solar neighbourhood. The probabilistic separation we propose can be extended to other data sets for which the accuracy in [a/Fe] is not sufficient to disentangle the chemical disc components a priori. For such data sets which will also have significant overlap with Gaia DR1, we can therefore make full use of the improved parallax and proper motion data as it becomes available to investigate kinematic trends in these chemical disc components.
Citation
Wojno, J., Kordopatis, G., Steinmetz, M., McMillan, P., Matijevič, G., Binney, J., Wyse, R. F. G., Boeche, C., Just, A., Grebel, E. K., Siebert, A., Bienaymé, O., Gibson, B. K., Zwitter, T., Bland-Hawthorn, J., Navarro, J. F., Parker, Q. A., Reid, W., Seabroke, G., & Watson, F. (2016). Chemical separation of disc components using RAVE. Monthly notices of the Royal Astronomical Society, 461(4), 4246-4255. https://doi.org/10.1093/mnras/stw1633
Acceptance Date | Jul 5, 2016 |
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Online Publication Date | Jul 7, 2016 |
Publication Date | Oct 1, 2016 |
Deposit Date | Dec 6, 2017 |
Publicly Available Date | Dec 6, 2017 |
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 | 461 |
Issue | 4 |
Pages | 4246-4255 |
DOI | https://doi.org/10.1093/mnras/stw1633 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://hull-repository.worktribe.com/output/496731 |
Publisher URL | https://academic.oup.com/mnras/article/461/4/4246/2608747 |
Contract Date | Jul 7, 2016 |
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Copyright Statement
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
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