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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 5.

Observed position (left), proper motion (middle), and acceleration (right) uncertainties as a function of projected radius. The average uncertainty along the X and Y coordinates are plotted. The filled circles mark the stars in our narrow-field data set and unfilled squares indicate the stars in the wide-field mosaic data, which have projected radii R > 5''.

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