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Table 4

Parameters used to simulate synthetic spectra of rMS and bMS stars and estimation of helium difference between the two population for different ICUT in the case of NGC 6121.

I CUT T EFF,bMS T EFF,rMS log gbMS log grMS ΔY

17.3 5542 5571 4.58 4.57 0.014
17.5 5397 5444 4.60 4.60 0.021
17.7 5247 5297 4.63 4.63 0.022
17.9 5095 5149 4.65 4.65 0.024
18.1 4944 4989 4.66 4.66 0.021

Average 0.020, σ = 0.008

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