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Table 1.

Stellar properties of the CHE and standard Pop III models, at the start and end of the MS.

Mass Teff(Xc = 0.75 → 0) Tc(Xc = 0.75 → 0) L(Xc = 0.75 → 0) R(Xc = 0.75 → 0) τMS Nγ(HII)(1) Nγ(HeII) (1) Nγ(HeIII) (1) Nγ(LW) (1)
M log10[K] log10[K] log10[L] R Myr
9 CHE 4.68 → 4.86 7.86 → 7.86 3.96 → 5.17 1.41 → 2.46 27.15 8.08 × 1062 3.00 × 1062 4.54 × 1060 2.98 × 1062
9 standard 4.63 → 4.60 7.86 → 8.08 3.72 → 4.08 1.31 → 2.26 17.73 2.00 × 1062 3.20 × 1061 5.14 × 1058 1.02 × 1062
12 CHE 4.71 → 4.88 7.88 → 7.88 4.30 → 5.39 1.76 → 2.86 17.45 1.55 × 1063 6.69 × 1062 1.32 × 1061 5.37 × 1062
12 standard 4.67 → 4.64 7.85 → 8.11 4.11 → 4.46 1.75 → 3.03 17.86 4.96 × 1062 1.11 × 1062 4.21 × 1059 2.21 × 1062
15 CHE 4.76 → 4.91 7.93 → 7.93 4.56 → 5.55 1.92 → 2.96 12.83 2.43 × 1063 1.26 × 1063 3.56 × 1061 7.77 × 1062
15 standard 4.73 → 4.66 7.93 → 8.12 4.33 → 4.71 1.68 → 3.63 13.00 9.09 × 1062 2.63 × 1062 1.84 × 1060 3.65 × 1062
20 CHE 4.81 → 4.95 7.99 → 7.99 4.87 → 5.75 2.16 → 3.11 9.07 4.10 × 1063 2.63 × 1063 1.10 × 1062 1.20 × 1063
20 standard 4.79 → 4.68 7.99 → 8.14 4.66 → 5.04 1.83 → 4.69 9.52 1.89 × 1063 7.07 × 1062 9.25 × 1060 6.84 × 1062
30 CHE 4.87 → 4.99 8.04 → 8.04 5.27 → 6.00 2.66 → 3.53 6.11 8.01 × 1063 6.22 × 1063 3.81 × 1062 2.17 × 1063
30 standard 4.86 → 4.71 8.04 → 8.17 5.09 → 5.44 2.19 → 6.51 6.13 4.66 × 1063 2.28 × 1063 5.51 × 1061 1.52 × 1063
40 CHE 4.89 → 5.00 8.06 → 8.06 5.52 → 6.17 3.17 → 4.01 4.89 1.25 × 1064 1.06 × 1064 7.61 × 1062 3.28 × 1063
40 standard 4.90 → 4.73 8.06 → 8.18 5.37 → 5.69 2.57 → 8.17 4.78 8.23 × 1063 4.65 × 1063 1.55 × 1062 2.55 × 1063
60 CHE 4.92 → 5.02 8.08 → 8.08 5.84 → 6.40 4.05 → 4.86 3.82 2.25 × 1064 2.08 × 1064 1.76 × 1063 5.72 × 1063
60 standard 4.94 → 4.73 8.08 → 8.19 5.73 → 6.00 3.24 → 11.51 3.67 1.68 × 1064 1.10 × 1064 5.23 × 1062 4.92 × 1063
85 CHE 4.94 → 5.03 8.09 → 8.09 6.09 → 6.59 4.98 → 5.75 3.25 3.61 × 1064 3.52 × 1064 3.32 × 1063 8.96 × 1063
85 standard 4.96 → 4.73 8.09 → 8.20 6.00 → 6.23 3.97 → 15.20 3.08 2.90 × 1064 2.09 × 1064 1.23 × 1063 8.22 × 1063
120 CHE 4.95 → 5.03 8.10 → 8.10 6.32 → 6.77 6.09 → 6.84 2.86 5.63 × 1064 5.72 × 1064 5.81 × 1063 1.38 × 1064
120 standard 4.98 → 4.72 8.10 → 8.21 6.25 → 6.44 4.89 → 20.27 2.74 4.78 × 1064 3.69 × 1064 2.53 × 1063 1.33 × 1064
180 CHE 4.95 → 5.03 8.09 → 8.09 6.57 → 6.97 7.91 → 8.66 2.54 9.48 × 1064 9.72 × 1064 1.00 × 1064 2.31 × 1064
180 standard 4.99 → 4.52 8.09 → 8.23 6.51 → 6.68 6.40 → 65.09 2.88 8.35 × 1064 6.57 × 1064 5.15 × 1063 2.41 × 1064
250 CHE 4.96 → 5.04 8.09 → 8.09 6.75 → 7.13 9.60 → 10.35 2.36 1.41 × 1065 1.47 × 1065 1.55 × 1064 3.42 × 1064
250 standard 4.99 → 4.33 8.09 → 8.23 6.72 → 6.86 7.92 → 195.50 3.08 1.27 × 1065 1.02 × 1065 8.51 × 1063 3.71 × 1064
300 CHE 4.96 → 5.04 8.09 → 8.09 6.85 → 7.22 10.54 → 11.28 2.27 1.74 × 1065 1.83 × 1065 2.00 × 1064 4.19 × 1064
300 standard 4.99 → 4.01 8.09 → 8.23 6.82 → 6.95 8.80 → 905.61 3.01 1.57 × 1065 1.28 × 1065 1.10 × 1064 4.63 × 1064

Notes.

(1)

Nγλ) refers to the number of photons emitted in the wavelength range Δλ, integrated over the whole (MS) lifetime of the considered star: Nγλ,m) = ∫γλ,t,m)dt.

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