**Table 6:** Line fluxes^a for W 3 IRS5.
$\begin{table} \par\begin{displaymath} \begin{array}{p{0.32\linewidth}cccccc} \... ...0.33\\ \noalign{\smallskip } \hline \end{array} \end{displaymath}\end{table}$

a(b) means $a\times10^b$ .
^a The line fluxes are given in W cm^-2 $\mu$ m^-1, except for the 538.3 $\mu$ m line observed with SWAS, for which the integrated intensity
in K km s^-1 is listed. To convert to W cm^-2, multiply by $\Delta \lambda = \lambda/R$ in $\mu$ m, with $R\approx 9200$ . A negative value indicates absorption.
^b The upper limits are 3 $\sigma$ values.
^c Tentative detection at the $\sim$ 3 $\sigma$ level, due to shifted wavelength of absorption feature (see Fig. 1).

Source LaTeX | All tables | In the text