Table 1
SSCs within the area observed with SINFONI.
| SSC | Agea | Mass | Ref.b | Flux H2 | Flux Brγ |
| ID | Myr | 106M⊙ | erg s-1 cm-2 | ||
|
|
|||||
| D | 3.9 | 1.4 | [1] | <2.9 × 10-16 | 2.1 ± 0.1 × 10-15 |
| 30 | 1.45 | 0.32 | [2] | ||
|
|
|||||
| D1 | 6.1 | 1.6 | [1] | <1.1 × 10-16 | <1.5 × 10-16 |
| 3 | – | – | [2] | ||
|
|
|||||
| D2 | 5.4 | 0.8 | [1] | <1.1 × 10-16 | 6.7 ± 0.3 × 10-16 |
|
|
|||||
| C | 5.7 | 4.1 | [1] | <1.0 × 10-16 | <9.9 × 10-17 |
| 28 | 4.8 | 1.2 | [2] | ||
|
|
|||||
| B1c | 3.5 | 4.2 | [1] | 2.9 ± 0.2 × 10-15 | 2.2 ± 0.1 × 10-14 |
| 16 | 1 | 6.8 | [2] | ||
Notes. Fluxes are not corrected for extinction. Masses estimated by Gilbert & Graham (2007) are not corrected by extinction.
Errors in ages estimated by Gilbert & Graham (2007) are derived from Starburst99 fits to the Brγ EW and are typically below 0.1 Myr. Cluster D2 has a larger error on the Brγ EW, the error on the age is 5.4
.
[1] Gilbert & Graham (2007), [2] Table 8 in Whitmore et al. (2010).
SSC first identified by Whitmore & Schweizer (1995) as WS80.
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