Table 7
Properties of the globulettes as derived from background stars.
| RN | A V | n(H2) | M NIR | M OPT |
| (mag) | (104 cm-3) | (MJup) | (MJup) | |
|
|
||||
| 33 | 0.9 | 0.8 | 18.6 | 12.7 |
| 35 | 8.4 | 2.8 | 1164 | 172 |
| 1.9 | − | − | − | |
| 52 | 8.6 | 4.5 | 504 | 34.7 |
| 54 | 1.6 | 1.8 | 18.6 | 5.1 |
| 55 | 4.5 | 1.5 | 514 | 67.2 |
| F14−west2 | 7.5 | 2.6 | − | − |
| F14−west3 | 6.4 | 2.2 | − | − |
| F14−west4 | 2.4 | 0.8 | − | − |
| F14−west5 | 1.2 | 0.4 | − | − |
| F14−east | 10.2 | 2: | − | − |
| F15−tip | 14.2 | 4: | − | − |
Notes. The first column lists the globulette ID. The second column is the AV caused by globulettes and trunks. Columns 3 and 4 are the calculated number density and the mass. The last six entries refer to stars behind the densest trunks. Column 5 contains the optically derived masses by G07.
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