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Identifying Multiple Populations in M71 Using CN

  • Authors: Jeffrey M. Gerber, Eileen D. Friel, and Enrico Vesperini

2020 The Astronomical Journal 159 50.

  • Provider: AAS Journals

Caption: Figure 5.

CH(4300) band strength against effective temperature. Our measurements for M10 from G18 are shown on the left panel, and the results from this work for M71 are on the right. RGB stars are shown as black points and AGB stars are shown as red stars.

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