The helium mass fraction difference between the two main populations of NGC 2808 is about 0.15, the same as inferred without chemically self-consistent models.
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Chemically Self-Consistent Modeling of the Globular Cluster NGC 2808 and its Effects on the Inferred Helium Abundance of Multiple Stellar Populations
The helium mass fraction difference between the two main populations of NGC 2808 is about 0.15, the same as inferred without chemically self-consistent models.