Figure 4 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 4.

Error analysis of the radial asymmetrical structures in the R, Z plane for Figure 3, with each panel showing bootstrap errors for the corresponding quantities in each bin of Figure 3. Most of the value is from 5 to 10 km s⁻¹ with blue color and some values can reach 15–20 km s⁻¹ with red color.

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