All Tables

Table 1: Results from fitting a single reddened blackbody to the K- and L-band spectra. In addition to the blackbody temperature and the K-band extinction obtained from the fitting procedure, we list the L-band magnitudes ( $\pm$ 0.2 mag uncertainty) we derived from our images.
Table 2: The optical depths of the 4 absorption features at $3.0~{\mu}$ m, $3.4~\mu$ m and $3.48~\mu$ m.
Table 3: Diagnostic line ratios for the three IRS 16 sources in common with Najarro et al. (1997).
Table 4: Continuum and emission line strengths as well as linewidths and equivalent widths of the Br $\alpha$ line towards the observed sources.
Table 5: Continuum and emission line strengths as well as linewidths and equivalent widths of the Pf $\gamma$ line towards the observed sources.
Table 6: Continuum and emission line strengths as well as linewidths and equivalent widths of the Pf $\delta$ line towards the observed sources.