Figure 6 from Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. III. A New Velocity Substructure and Time Stamps of the Galactic Disk Asymmetry in the Disk between 12 and 15 kpc

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Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. III. A New Velocity Substructure and Time Stamps of the Galactic Disk Asymmetry in the Disk between 12 and 15 kpc

Authors: Hai-Feng Wang, Jeffrey L. Carlin, Y. Huang, Martíin López-Corredoira, B.-Q. Chen, C. Wang, J. Chang, H.-W. Zhang, M.-S. Xiang, H.-B. Yuan, W.-X. Sun, X.-Y. Li, Y. Yang, and L.-C. Deng

2019 The Astrophysical Journal 884 135.

Provider: AAS Journals

Caption: Figure 6.

Similar to Figure 4, but for the error analysis of the rotational (V_θ) asymmetrical structures in the R, Z plane of the LAMOST-Gaia stars in different age populations. Most of the bins values are small with blue color, accompanied by some redder bins belonging to 10–15 km s⁻¹.

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