Table 3: Relative line fluxes.
  I II III IV V VI VII

Line (Å)
F F F F F F F
4861 H$\beta$ - 9 (3) 15 (4) - 20 (8) 18 (5) -
6300 [O I] 17 (6) 17 (9) 9 (3) - - - 30 (6)
6548 [N II] 20 (7) 15 (6) 15 (6) 14 (5) 14 (7) 13 (6) 16 (3)
6563 H$\alpha $ 100 (33) 100 (46) 100 (37) 100 (33) 100 (49) 100 (43) 100 (19)
6584 [N II] 65 (21) 44 (20) 44 (16) 50 (17) 46 (23) 53 (22) 52 (10)
6716 [S II] 59 (20) 48 (23) 38 (15) 27 (9) 26 (13) 31 (12) 45 (9)
6731 [S II] 48 (17) 34 (16) 26 (11) 20(7) 20 (10) 22 (9) 34 (7)

Absolute H$\alpha $ flux$^{\rm 1}$
6.5 12.8 15.5 10.5 13.5 6.5 5.7
H$\alpha $/H$\beta$ - 11 (3) 7 (4) - 5.0 (8) 5.5 (5) -
[S II]/H$\alpha $ 1.08 (20) 0.83 (24) 0.64 (16) 0.47 (11) 0.46 (16) 0.53 (14) 0.80 (10)
I(6716)/I(6731) 1.23 (13) 1.41 (13) 1.45 (9) 1.37 (6) 1.30 (8) 1.36 (7) 1.31 (6)
n$_{\rm e}$$^{\rm 2}$ <380 cm-3 <120 cm-3 <130 cm-3 <320 cm-3 <330 cm-3 <290 cm-3 <410 cm-3
$^{\rm 1}$ In units of 10-17 erg s-1 cm-2 arcsec-2.
$^{\rm 2}$ 1$\sigma$ upper limits.
All fluxes are not corrected for interstellar extinction Numbers in parentheses represent the signal-to-noise ratio of the quoted values All fluxes normalized to F(H$\alpha $)=100.

Source LaTeX | All tables | In the text