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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 7.

(a) Upper CMD of proper motion probable members (Pμ ⩾ 19%) from P11 with blue HB candidates highlighted in blue diamonds. Small light gray points are stars with Pμ < 19%. (b) CMD, including radial velocity membership determinations. Single members (SMs) are shown as black points, circled points indicate binary likely members (BLMs). Gray points are SMs and BLMs with 1% ⩽ Pμ < 19%. Gray "⊗" symbols mark candidate binary members currently classified as binary unknowns (BUs) or binary likely non-members (BLNs), discussed in Section 6.1.

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