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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 21.

Left: density of normal vectors for the B stars (K ⩾ 14) in our sample. The peak density, 0.002 stars deg −2, is located at ( i, Ω) = (136°, 85°). Right: density of normal vectors for an isotropically distributed sample of 18 stars. The same stretch is used for both density maps.

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