Figure 4 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.

Caption: Figure 4.

Residuals in X (left) and Y (right) after subtracting the best-fit acceleration curves shown in Figure 3 for each of the six accelerating sources.