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Table 5

Parameters used to simulate synthetic spectra of MSa and MSbc stars and estimation of helium difference between the two population for different ICUT in the case of NGC 6752.

I CUT T EFF,MSa T EFF,MSbc log gMSa log gMSbc ΔY

18.55 5410 5456 4.65 4.65 0.021
18.75 5254 5306 4.67 4.67 0.023
18.95 5100 5150 4.69 4.69 0.023
19.15 4946 4998 4.70 4.70 0.025
19.35 4798 4851 4.72 4.72 0.026

Average 0.024, σ = 0.006

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