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• W2790068007 abstract "There are multiple groups of comoving stars in the Solar neighbourhood, which are possible signatures of one of the fundamental resonances of non-axisymmetric structure such as the Galactic bar or spiral arms. One such stream, Hercules, has been proposed to result from the outer Lindblad resonance of a short-fast rotating bar as shown analytically, or the corotation resonance of a longer slower rotating bar as observed in an N-body model. We show that by including an m = 4 Fourier component in an analytical long bar model, with an amplitude that is typical for bars in N-body simulations, we can reproduce a Hercules-like feature in the stellar kinematics of the Solar neighbourhood. We describe the expected symmetry in the velocity distribution arising from such a model, which we will soon be able to test with Gaia." @default.
• W2790068007 created "2018-03-29" @default.
• W2790068007 creator A5024961741 @default.
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• W2790068007 date "2018-04-16" @default.
• W2790068007 modified "2023-10-17" @default.
• W2790068007 title "The 4:1 outer Lindblad resonance of a long-slow bar as an explanation for the Hercules stream" @default.
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• W2790068007 doi "https://doi.org/10.1093/mnras/sty921" @default.
• W2790068007 hasPublicationYear "2018" @default.
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