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The Kinematics and Chemistry of Red Horizontal Branch Stars in the Sagittarius Streams

  • Authors: W. B. Shi, Y. Q. Chen, K. Carrell, and G. Zhao

Shi et al. 2012 The Astrophysical Journal 751 130.

  • Provider: AAS Journals

Caption: Figure 10.

Left panel: radial velocity as a function of longitude of the Sgr orbital plane for our RHB stars. The polynomial fit to the distribution is also plotted. Right panel: distribution of the differences between the polynomial fit and the data. A Gaussian fit is also shown.

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