Image Details

Choose export citation format:

WIYN Open Cluster Study. LIX. Radial Velocity Membership of the Evolved Population of the Old Open Cluster NGC 6791

  • Authors: Benjamin M. Tofflemire, Natalie M. Gosnell, Robert D. Mathieu, and Imants Platais

Tofflemire et al. 2014 The Astronomical Journal 148 61.

  • Provider: AAS Journals

Caption: Figure 6.

Comparison of the P11 Pμ values (y axis) with our PRV values (x axis) for single stars. The dashed vertical line represents the radial velocity membership criterion (50%). The blue HB candidates from P11 are highlighted in blue diamonds. Blue diamonds without a central point are velocity variable. Their radial velocity membership position reflects the membership probability of their mean radial velocity. Marginal distributions along each axis are presented in the top and right panels.

Other Images in This Article
Copyright and Terms & Conditions