Skip to main content

Research Repository

Advanced Search

The rich are different: evidence from the RAVE survey for stellar radial migration

Kordopatis, G.; Binney, J.; Gilmore, G.; Wyse, R. F. G.; Belokurov, V.; McMillan, P. J.; Hatfield, P.; Grebel, E. K.; Steinmetz, M.; Navarro, J. F.; Seabroke, G.; Minchev, I.; Chiappini, C.; Bienaymé, O.; Bland-Hawthorn, J.; Freeman, K. C.; Gibson, B. K.; Helmi, A.; Munari, U.; Parker, Q.; Reid, W. A.; Siebert, A.; Siviero, A.; Zwitter, T.

Authors

G. Kordopatis

J. Binney

G. Gilmore

R. F. G. Wyse

V. Belokurov

P. J. McMillan

P. Hatfield

E. K. Grebel

M. Steinmetz

J. F. Navarro

G. Seabroke

I. Minchev

C. Chiappini

O. Bienaymé

J. Bland-Hawthorn

K. C. Freeman

B. K. Gibson

A. Helmi

U. Munari

Q. Parker

W. A. Reid

A. Siebert

A. Siviero

T. Zwitter



Abstract

Using the RAdial Velocity Experiment fourth data release (RAVE DR4), and a new metallicity calibration that will be also taken into account in the future RAVE DR5, we investigate the existence and the properties of super-solar metallicity stars ([M/H] ≳ +0.1dex) in the sample, and in particular in the Solar neighbourhood. We find that RAVE is rich in super-solar metallicity stars, and that the local metallicity distribution function declines remarkably slowly up to +0.4dex. Our results show that the kinematics and height distributions of the super-solar metallicity stars are identical to those of the [M/H] ≲ 0 thin-disc giants that we presume were locally manufactured. The eccentricities of the super-solar metallicity stars indicate that half of them are on a roughly circular orbit (e ≤ 0.15), so under the assumption that the metallicity of the interstellar medium at a given radius never decreases with time, they must have increased their angular momenta by scattering at corotation resonances of spiral arms from regions far inside the Solar annulus. The likelihood that a star will migrate radially does not seem to decrease significantly with increasing amplitude of vertical oscillations within range of oscillation amplitudes encountered in the disc.

Citation

Kordopatis, G., Binney, J., Gilmore, G., Wyse, R. F. G., Belokurov, V., McMillan, P. J., …Zwitter, T. (2015). The rich are different: evidence from the RAVE survey for stellar radial migration. Monthly notices of the Royal Astronomical Society, 447(4), 3526-3535. https://doi.org/10.1093/mnras/stu2726

Journal Article Type Article
Acceptance Date Dec 19, 2014
Online Publication Date Jan 24, 2015
Publication Date Mar 11, 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 4
Pages 3526-3535
DOI https://doi.org/10.1093/mnras/stu2726
Keywords Galaxy : abundances; Galaxy : disc; Galaxy : evolution; Galaxy : kinematics and dynamics; Galaxy : stellar content
Public URL https://hull-repository.worktribe.com/output/543562
Publisher URL https://academic.oup.com/mnras/article/447/4/3526/1752326

Files






You might also like



Downloadable Citations