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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 19.

Normalized distribution of K-band luminosities of the most likely members (see Appendix E) of the disk (red solid) and the remaining stars (black dashed). A two-sample KS test yields a probability of 87% that the most likely disk members have the same KLF as the remainder of the sample. We caution that the K-band magnitudes in this figure are observed magnitudes and have not been corrected for completeness or extinction effects.

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