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. 2000 Apr 4;97(9):4551–4555. doi: 10.1073/pnas.070590597

Table 1.

Summary of [Cl iii] observations

Object Observation date I(5518 Å) I(5538 Å) I(8434 Å) I(8481 Å) I(8500 Å) C*
NGC 2440 Nov. 18, 1989 5.40−1 6.21−1 9.00−2 0.53
NGC 6537 June 15, 1992 3.85−1 9.16−1 1.91−2 1.80
NGC 6572 Aug. 5, 1990 1.58−1 3.75−1 1.50−2 1.70−2 2.10−2 0.40
NGC 6572 Sept. 1, 1991 1.70−1 3.97−1 2.10−2 2.40−2 3.10−2 0.40
NGC 6741 Sept. 30, 1991 6.32−1 1.02+0 3.80−2 6.40−2 1.10
NGC 6884 Aug. 30, 1994 2.73−1 4.99−1 4.50−2 1.10
NGC 7009 July 27, 1988 2.97−1 4.08−1 2.90−2 2.50−2 0.08
NGC 7027 Sept. 4, 1987 1.67−1 6.37−1 8.60−2 7.10−2 8.60−2 1.37
NGC 7662 Aug. 28, 1988 2.70−1 3.35−1 5.70−2 0.10
IC 2165 Nov. 17, 1989 3.30−1 3.70−1 3.00−2 4.00−2 0.68
IC 4997 Aug. 3, 1990 4.60−2 1.20−1 1.50−2 2.00−2 1.70−2 0.80
IC 4997 Aug. 30, 1991 6.10−2 1.31−1 1.30−2 3.30−2 2.80−2 0.80
Hubble 12 Aug. 6, 1990 5.00−2 1.35−1 6.00−2 6.20−2 6.40−2 1.35

Line intensities I (in energy units), corrected for interstellar extinction, are given relative to I(Hβ) = 100. A ± B implies A × 10±B

*

Interstellar extinction coefficient C = 1.47E(BV) = log[Ii(Hβ)/Io(Hβ)], where Ii(Hβ) and Io(Hβ) are the intrinsic and observed Hβ line intensities, respectively.