Table 6: Continuum and emission line strengths as well as linewidths and equivalent widths of the Pf$\delta $ line towards the observed sources.
Object Line-continuum of HI (3.296$~\mu$m) Integral of HI (3.296$~\mu$m) EW of HI (3.296$~\mu$m) Line width
    $ 10^{-18}~\rm W~cm^{-2}~\mu m^{-1}$   $10^{-18}~\rm W~cm^{-2}$ Å Å
IRS 1 W $ 7.80\pm0.20 ~$ $ 0.0573\pm0.0097$ $ -9.26\pm0.81~$  $147\pm21$
IRS 3 -   -   -   -
IRS 7 $ 12.00\pm2.00 ~$ $ 0.0450\pm0.0135$ $ -3.50\pm0.94~$  $75\pm10$
IRS 9 -   -   -   -
IRS 21 -   -   -   -
IRS 29 -   -   -   -
IRS 13 $4.80\pm0.20 ~$ $0.0226\pm0.0033$ $-7.65\pm0.68~$  $94\pm10$
IRS 13 N $ 3.30\pm0.30 ~$ $ 0.0208\pm0.0054$ $ -8.29\pm0.99~$  $126\pm21$
IRS 16 CC -   -   -   -
IRS 16 C $ 0.57\pm0.12 ~$ $0.0027\pm0.0008$ $ -7.57\pm1.19~$  $94\pm10$
IRS 16 NE $ 1.15\pm0.16 ~$ $0.0084\pm0.0024$ $ -7.62\pm1.31~$  $147\pm21$
IRS 16 SW $ 0.38\pm0.09 ~$ $0.0026\pm0.0008$ $ -4.30\pm1.18~$  $137\pm10$


Source LaTeX | All tables | In the text