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Table 1

Models that reproduce abundances calculated via collisional excited lines. The “W” and “S” are for well-mixed and selective wind prescription, respectively.

Model Mup wind Mgas t O/Ha log (C/O) log (N/O) log (Ne/O) log (S/O) log (Cl/O) log (Ar/O) log (Fe/O)
(M) (108 M) (Gyr)

M1C 60 8.99 13.50 7.95 –0.08 –0.44 –0.85 –1.63 –3.87 –2.45 –1.20
12.90 7.90 –0.08 –0.43 –0.85 –1.63 –3.87 –2.45 –1.20
7.50 7.68 –0.09 –0.39 –0.84 –1.63 –3.89 –2.44 –1.21

M2C 60 W 2.08 13.50 8.32 –0.15 –0.63 –0.88 –1.65 –3.81 –2.47 –1.20
12.90 8.25 –0.14 –0.61 –0.88 –1.65 –3.81 –2.46 –1.20
7.50 7.96 –0.17 –0.50 –0.87 –1.65 –3.84 –2.45 –1.21

M3C 60 W-S 2.08 13.50 8.19 –0.06 –0.52 –0.88 –1.63 –3.81 –2.46 –1.17
12.90 8.20 –0.14 –0.60 –0.88 –1.65 –3.82 –2.46 –1.20
7.50 7.96 –0.17 –0.50 –0.87 –1.65 –3.84 –2.45 –1.21

M4C 40 W 2.08 13.50 8.13 0.04 –0.40 –0.87 –1.45 –3.64 –2.27 –1.00
12.90 8.05 0.05 –0.37 –0.87 –1.45 –3.64 –2.27 –1.01
7.50 7.76 0.02 –0.27 –0.84 –1.43 –3.67 –2.26 –1.00

Observational constraints
H ii region, A stars 1.98b  ±  0.20 13.50 8.16c  ±  0.04 –1.61 ± 0.14 –0.72  ±  0.06 –1.61  ±  0.10 –3.69d ± 0.06 –2.20  ±  0.08 –1.15e  ±  0.20
PN young 12.90  ±  0.50 8.11  ±  0.10 –0.77  ±  0.14 –1.80  ±  0.20 –2.26 ± 0.16
PN old 7.50  ±  3.00 7.72  ±  0.10 –0.74  ±  0.16 –1.62  ±  0.20 –2.26  ±  0.16

Notes. 

(a)

Abundances in units of 12 + log (O/H).

(b)

CCP06.

(c)

Adding 0.08 dex to O gaseous value due to depletion in dust grains.

(d)

Peimbert et al.(2005).

(e)

Fe/H from A-stars by Venn et al. (2001) and CEL O/H from H ii regions.

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