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 (
0.2 mag uncertainty) we derived from our images.
| Source |
Blackbody |
AK |
L-band |
| |
temperature |
|
magnitude |
| IRS 1W |
900 |
3.30 |
5.8 |
| IRS 3 |
800 |
4.20 |
5.3 |
| IRS 7 |
2100 |
3.55 |
5.0 |
| IRS 9 |
1900 |
3.10 |
7.4 |
| IRS 21 |
1200 |
3.95 |
6.8 |
| IRS 29 |
1600 |
3.70 |
7.4 |
| IRS 16C |
22 600 |
3.45 |
8.6 |
| IRS 16CC |
20 200 |
4.00 |
9.0 |
| IRS 16NE |
22 400 |
3.25 |
7.7 |
| IRS 16SW |
22 500 |
3.25 |
8.4 |
| IRS 13 |
1300 |
3.00 |
6.7 |
| IRS 13N |
1000 |
3.90 |
9.76 |
Source LaTeX |
All tables |
In the text