Table 4: Continuum and emission line strengths as well as linewidths and equivalent widths of the Br$\alpha $ line towards the observed sources.
Object Line-continuum of HI (4.051$~\mu$m) Integral of HI (4.051$~\mu$m) EW of HI (4.051$~\mu$m) Line width
    $ 10^{-18}~\rm W~cm^{-2}~\mu m^{-1}$   $10^{-18}~\rm W~cm^{-2}$ Å Å
IRS 1 W $55.9\pm0.40~$ $ 0.5869\pm0.1216 ~$ $ -41.48\pm1.86~$  $210\pm42$
IRS 3 $5.80\pm0.50~$ $ 0.0855\pm0.0378 ~$ $ -6.02\pm2.83~$  $295\pm105$
IRS 7 -   -   -   -
IRS 9 $19.60\pm0.40~$ $ 0.1137\pm0.0121 ~$ $ -63.56\pm1.64~$  $116\pm10$
IRS 21 $13.00\pm0.20~$ $ 0.1566\pm0.0362 ~$ $ -48.03\pm1.90~$  $241\pm52$
IRS 29 $1.70\pm0.20~$ $ 0.0196\pm0.0041~$ $ -10.26\pm1.75~$  $231\pm21$
IRS 13 $47.50\pm0.40~$ $ 0.8479\pm0.0570 ~$ $ -87.59\pm2.63$  $357\pm21$
IRS 13 N $35.60\pm0.30~$ $ 0.2243\pm0.0393 ~$ $ -63.58\pm1.18~$  $126\pm21$
IRS 16 CC $1.69\pm0.03~$ $ 0.0275\pm0.0066 ~$ $ -58.20\pm4.39~$  $326\pm73$
IRS 16 C $3.86\pm0.06~$ $ 0.0588\pm0.0028 ~$ $ -117.43\pm3.28~$  $305\pm10$
IRS 16 NE $10.19\pm0.08$ $ 0.1126\pm0.0065$ $ -112.82\pm2.94~$  $221\pm11$
IRS 16 SW $6.29\pm0.07~$ $ 0.1025\pm0.0109~$ $ -120.66\pm3.61~$  $326\pm31$


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