Figure 1 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 1.

Left and right panels show the distribution in the R–Z plane of projected relative age and distance errors, respectively. The color bars indicate the relative age errors (left) and relative distance errors (right). The blue/cyan colors dominate the pattern implying that most of the relative age error is less than 38% and most of the relative distance error is less than 8%.

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