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Table 1:

Emission line fluxes for the H$\beta $, [O III]  $\lambda 5007$, H$\alpha $, [N II]  $\lambda 6583$ and the [S II] $\lambda \lambda 6716,6731$ lines as measured from Gaussian fits to the spectra of the region A to G.

Region 		H$\beta $ [O III] $~\lambda5007$ H$\alpha $ [N II] $~\lambda 6583$ [S II]  $\lambda 6716$ [S II]  $\lambda 6731$
  Line fluxes in units of $10^{-16}~{\rm erg}~{\rm s}^{-1}~{\rm cm}^{-2}$
A <0.5 $5.9\pm 0.2$ $1.9\pm 0.2$ $1.1\pm 0.1$ - -
B $1.0\pm 0.2$ $19.5\pm 0.3$ $4.1\pm 0.3$ $2.8\pm 0.3$ - -
C $7.2\pm 0.2$ $56.8\pm 0.4$ $21.7\pm 0.3$ $11.9\pm 0.3$ $4.7\pm 0.3$ $ 3.8\pm 0.3$
D $2.9\pm 0.4$ $8.5\pm 0.5$ $4.9\pm 0.5$ $4.2\pm 0.5$ - -
E $2.7\pm 0.4$ $32.0\pm 0.5$ $10.5\pm 0.4$ $6.1\pm 0.3$ - -
F $1.3\pm 0.1$ $9.0\pm 0.1$ $3.8\pm 0.2$ $2.0\pm 0.2$ - -
G (narrow) $5.7\pm 0.5$ $52.7\pm 1.7$ $19.1\pm 3.4$ $7.5\pm 2.3$ $2.8\pm 1.1$ $ 1.9\pm 0.9$
G (broad) $5.2\pm 0.6$ $29.9\pm 1.8$ $14.7\pm 2.5$ $10.6\pm 2.2$ $4.8\pm 1.2$ $ 4.5\pm 1.1$


Source LaTeX | All tables | In the text

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