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Table 6

Measured luminosities of the O I recombination lines of SN 2011dh at 99 and 198/202 days, and the corresponding factors derived from Eq. (3), using effective recombination coefficients cm3 s-1, cm3 s-1, cm3 s-1, cm3 s-1 (Appendix C), and ψ = 0.5.

Time
(days) (erg s-1(cm-3)) (erg s-1(cm-3)) (erg s-1(cm-3)) (erg s-1(cm-3))

99 1.8 × 1039 ( ≲ 2.8 × 108) 5.7 × 1038 ( ≲ 2.7 × 108) ... ...
198/202 1.6 × 1038 ( ≲ 2.9 × 107) 9.7 × 1037 ( ≲ 3.9 × 107) 6.5 × 1037 ( ≲ 2.7 × 107) 3.9 × 1037 (4.7 × 107)

Notes. Where the model calculations suggest line blending or scattering contributions, we add a symbol.

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