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Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3

Kawata, D; Baba, J; Hunt, JAS; Schönrich, R; Ciucǎ, I; Friske, J; Seabroke, G; (2021) Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3. Monthly Notices of the Royal Astronomical Society , 508 (1) pp. 728-736. 10.1093/mnras/stab2582. Green open access

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Abstract

Using a numerical simulation of an isolated barred disc galaxy, we first demonstrate that the resonances of the inner bar structure induce more prominent features in the action space distribution for the kinematically hotter stars, which are less sensitive to the local perturbation, such as the transient spiral arms. Then, we analyse the action distribution for the kinematically hotter stars selected from the Gaia EDR3 data as the stars with higher values of radial and vertical actions. We find several resonance features, including two new features, in the angular momentum distribution similar to what are seen in our numerical simulations. We show that the bar pattern speeds of about Ωbar ∼ 34 and 42 km s−1 kpc−1 explain all these features equally well. The resonance features we find correspond to the inner 4:1, co-rotation (CR), outer 4:1, outer Lindblad, and outer 4:3 (CR, outer 4:1, outer Lindblad, outer 4:3, and outer 1:1) resonances, when Ωbar ∼ 34 (42) km s−1 kpc−1 is assumed.

Type: Article
Title: Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stab2582
Publisher version: http://dx.doi.org/10.1093/mnras/stab2582
Language: English
Additional information: © 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: Galaxy: disc, Galaxy: evolution, Galaxy: kinematics and dynamics
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10135347
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