Figure 3 from TRIANGULUM II: A VERY METAL-POOR AND DYNAMICALLY HOT STELLAR SYSTEM

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

TRIANGULUM II: A VERY METAL-POOR AND DYNAMICALLY HOT STELLAR SYSTEM

Authors: Nicolas F. Martin, Rodrigo A. Ibata, Michelle L. M. Collins, R. Michael Rich, Eric F. Bell, Annette M. N. Ferguson, Benjamin P. M. Laevens, Hans-Walter Rix, Scott C. Chapman, and Andreas Koch

2016 The Astrophysical Journal 818 40.

Provider: AAS Journals

Caption: Figure 3.

Velocities of Tri II member stars as a function of their distance from the system’s centroid, showing an apparent flaring of the radial velocity distribution with distance. The hashed regions correspond to the velocities within ﹩\pm {\sigma }_{\mathrm{vr}}﹩ for the full sample (gray), the inner sample (blue), and the outer sample (red).

Other Images in This Article

Copyright and Terms & Conditions