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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 3.

δCN(4216) versus δS(3839) for the RGB stars in our sample. RGB stars with Teff > 5300 K are indicated as open circles. Histograms for each axis are shown with fits based on Gaussian Mixture Models overplotted.

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