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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 10.

HST UV photometry for M71 using the pseudo-CMD as seen in Milone et al. (2017). Stars from our sample are indicated with RGB stars as circles, AGB stars as stars, and HB stars as squares. All stars in common with this study are color-coded based on δCN(4216) value.

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