Open Access
Table F.1.
(Lbol, Ṁ)-relation for each cluster derived when fitting Eq. 5 to the (Lbol, ṀSED) measurements of the four clusters and the (Lbol, ṀCO) values for RSGC1. The MC method yields a best-fit slope b = 3.38
and intercept a2 for NGC 2100 of −21.75
.
| Cluster | difference in intercept (Δai) |
|---|---|
| Eq. (5) | |
| RSGC1 | −2.32 |
| NGC 2100 | 0 |
| NGC 7419 | −0.47 |
| χ Per | −0.33 |
| RSGC1 (CO) | −2.02 |
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