Figure 12 from Properties of the Remnant Clockwise Disk of Young Stars in the Galactic Center

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 12.

Left: eccentricity distribution of the clockwise disk. All orbital solutions falling within 15 fdg 2 of the disk are included, thereby weighting the distributions by disk membership probability. Right: eccentricity distributions shown separately for likely disk members with acceleration detections (solid) and without (dashed).

Other Images in This Article

Copyright and Terms & Conditions