Table 4: Results from emission line measurements. H  I measurements are performed on the difference spectrum (see text and Fig. 5). The H  I component at $14.5~{\rm ~ km ~ {s}^{-1}}$ is not detected in absorption and is probably due to background gas situated behind the star HD 102065.

Species		 $ V_{\rm LSR}~({\rm {km~ s}^{-1}}) $ $ T_{\rm b}~{\rm (K)}$ $FWHM~~({\rm {km~ s}^{-1}})$ $b~~({\rm {km~ s}^{-1}})$ $ N~~({\rm {cm}^{-2}})$

H  I   21 cm difference)		 $14.5\pm0.6$ $0.9\pm0.15$ $7.3\pm1.4$ $4.4\pm0.8$ $1.3\pm0.2\times 10^{19}$
  $4.2\pm0.1$ $20.4\pm1.1$ $3.2\pm0.2$ $1.9\pm0.1$ $1.3\pm0.07\times 10^{20}$
  $0.1\pm0.1$ $13.4\pm0.7$ $4.3\pm0.3$ $2.6\pm0.2$ $1.1\pm0.06\times 10^{20}$
  $-17.5\pm0.6$ $1.0\pm0.07$ $16\pm1.4$ $9.4\pm0.8$ $3.0\pm0.2\times 10^{19}$
CO(1-0) $2.8\pm0.2$ $7.0\times10^{-2}$ $3.5\pm0.3$ $2.1\pm 0.2$ $6.9\times 10^{13} ~ (J = 1)$
CO(2-1) $2.75\pm0.17$ $3.6\times 10^{-2}$ $3.0\pm0.3$ $1.8\pm0.2$ $1.8\times10^{13} ~ (J = 2)$
    $I~({\rm erg~ s}^{-1}~{\rm cm}^{-2}~{\rm sr}^{-1})$     N( C  II*)
${\rm C^{+}~ 158~\mu m}$ - $2.8\times10^{-6}$ - - $1.2\times10^{15}$


Source LaTeX | All tables | In the text