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Properties of the Remnant Clockwise Disk of Young Stars in the Galactic Center

  • Authors: S. Yelda, A. M. Ghez, J. R. Lu, T. Do, L. Meyer, M. R. Morris, and K. Matthews

Yelda et al. 2014 The Astrophysical Journal 783 131.

  • Provider: AAS Journals

Caption: Figure 7.

Left: line-of-sight velocity uncertainties plotted against K magnitude for the Keck/OSIRIS (red squares) and VLT/SINFONI (black circles) measurements. Right: comparison of radial velocity measurements for the 15 common stars in the two data sets.

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