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Orion OB1: B-type stars vs nebular (M42) abundances<br />
Elem.<br />
O<br />
O (g+d)<br />
C<br />
N<br />
Ne<br />
S<br />
Ar<br />
B-type stars<br />
(OriOB1)<br />
8.74 ± 0.04 †<br />
8.35 ± 0.03 †<br />
7.82 ± 0.07 †<br />
8.09 ± 0.05 †<br />
7.15 ± 0.05 ††<br />
6.66 ± 0.06 †††<br />
CEL<br />
8.51 ± 0.03<br />
8.64 – 8.67<br />
---<br />
7.65 ± 0.09<br />
7.78 ± 0.07<br />
7.06 ± 0.04<br />
6.50 ± 0.05<br />
M42 (E02)<br />
† Simón-Díaz (2010) + Nieva & Simón-Díaz (2011)<br />
†† Daflon et al. (2009)<br />
††† Lanz et al. (2008)<br />
8.42 ± 0.02<br />
8.16 ± 0.2<br />
7.92 ± 0.09 (b)<br />
6.87 ± 0.05 (b)<br />
(a) Classical icf<br />
(b) icf own model<br />
E02: Esteban et al. (2002)<br />
S-DS11: Simón-Díaz & Stasinska (2011) Rubin et al. (2010): IR[NeII] + IR[NeIII] = 8.01 ± 0.01 dex<br />
ORL<br />
8.63 ± 0.03<br />
8.72 – 8.77<br />
---<br />
---<br />
---<br />
CEL<br />
8.52 ± 0.01<br />
8.65 - 8.68<br />
---<br />
7.68 ± 0.10 (a)<br />
7.84 ± 0.03 (a)<br />
8.05 ± 0.03 (b)<br />
6.39 ± 0.03 (b)<br />
M42 (S-DS11)<br />
ORL<br />
8.65 ± 0.03<br />
8.74 – 8.79<br />
8.37 ± 0.03<br />
---<br />
8.03 ± 0.26 (a)<br />
8.25 ± 0.35 (b)<br />
---<br />
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