Table 9: Information on the extra nine Galactic sources taken from Martín-Hernández et al. (2002a) (see Sect. 5.4).
Source $R_{\rm Gal}$ R $A_{\rm K}$$^\dagger$ Ne/H$^\flat$ S/H$^\flat$ Ar/H$^\flat$ log $N_{\rm Lyc}^\ddagger$
  (kpc) (kpc)   ( $\times 10^{-4}$) ( $\times 10^{-5}$) ( $\times 10^{-6}$)  
IRAS 02219+6125 11.0 3.3 $1.5 \pm 0.5$ $1.4 \pm 0.3$ $0.6 \pm 0.2$ $2.6\pm0.7$ 49.2
IRAS 17455-2800 0.2 8.3 $1.8 \pm 0.2 $ $1.4 \pm 0.3$ $0.9 \pm 0.2$ $3.9\pm0.5$ 48.7
IRAS 18116-1646 4.3 4.5 $1.2 \pm 0.3$ $1.9 \pm 0.4$ $ 1.3 \pm 0.3 $ $6.8\pm0.9$ 48.6
IRAS 18317-0757 4.5 4.9 $2.0 \pm 0.3$ $1.8 \pm 0.4$ $0.9 \pm 0.2$ $4.6\pm0.7$ 48.2
IRAS 18434-0242 4.6 5.7 $1.6 \pm 0.2$ $1.8 \pm 0.4$ $0.5 \pm 0.1$ $4.0\pm0.6$ 48.6
IRAS 18502+0051 4.7 7.1 $2.2 \pm 0.2$ $1.9 \pm 0.4$ $0.7 \pm 0.1$ $3.1\pm0.4$ 48.5
IRAS 21190+5140 12.7 8.9 <0.1$^\lhd$ $1.0\pm0.2$ $0.32\pm0.05$ $1.9\pm0.2$ 48.6
IRAS 22308+5812 11.3 5.5 <0.1$^\lhd$ $0.9 \pm 0.2$ $0.5 \pm 0.1$ $3.5\pm0.7$ 48.0
IRAS 23030+5958 11.4 5.2 <0.3$^\lhd$ $1.5 \pm 0.2$ $1.1 \pm 0.2$ $3.0\pm0.3$ 48.4
$^\dagger$ K band extinction calculated from the Br$\beta $/Br$\alpha $ decrement. $^\flat$ Elemental abundance corrected for extinction and $T_{\rm e}$ variations.
$^\ddagger$ Lyman continuum flux from Martín-Hernández et al. (2002a). $^\lhd$ Taken as 0.

Source LaTeX | All tables | In the text