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Table 3

Optical emission lines of LEDA 84274 and IRAS 01250+2832.

Name Obs. wave.a Flux Obs. EWb Ratio with Hαc Ratio with Hαd
(Å) (10-16 erg   s-1   cm-2) (Å) This work Kim et al. (1995)

LEDA 84274

 [O iI]  3870 317.0 ± 1.9 54.6 ± 0.3 0.58 0.30
Hγ 4504 46.5 ± 1.4 7.4 ± 0.2 0.08 ...
Hβ 5045 120.5 ± 1.1 20.6 ± 0.2 0.22 0.18
 [O iii 5146 81.9 ± 1.1 13.5 ± 0.2 0.15 0.12
 [O iii 5196 240.0 ± 1.1 40.6 ± 0.2 0.44 0.37
HeI 6094 18.8 ± 0.5 3.2 ± 0.1 0.03 ...
 [O i 6536 23.0 ± 0.4 4.4 ± 0.1 0.04 0.04
 [O i 6603 8.5 ± 0.4 1.6 ± 0.1 0.02 ...
 [N ii 6794 61.1 ± 0.6 11.8 ± 0.1 0.11 0.10
Hα 6808 549.0 ± 0.5 106.1 ± 0.1 1.00 1.00
 [N ii 6830 178.0 ± 0.5 34.6 ± 0.1 0.32 0.31
 [S ii 6968 78.9 ± 0.4 15.5 ± 0.1 0.14 0.14
 [S ii 6983 65.1 ± 0.4 12.8 ± 0.1 0.12 0.11

IRAS 01250+2832

 [N ii 6828 4.3 ± 0.8 1.5 ± 0.3 1.02 ...
Hα 6844 4.2 ± 0.8 1.4 ± 0.3 1.00 ...
 [N ii 6864 12.1 ± 0.8 4.2 ± 0.3 2.88 ...

Notes. 

(a)

Observed wavelength. A typical error of measurements is less than 1 Å.

(b)

Observed equivalent width.

(c)

Emission line ratio with Hα in this work. A typical measurement error is less than 0.01.

(d)

Emission line ratio with Hα in Kim et al. (1995).

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