Distribution of stars in different mass ranges along with the percentage of confidence level in the mass-segregation effect for the clusters.
| Object . | Mass range . | Confidence level . |
|---|---|---|
| . | (M⊙) . | (percentage) . |
| NGC 5617 | 4.0−2.4, 2.4−1.2, 1.2−0.8 | 88 |
| Trumpler 22 | 4.1−2.6, 2.6−1.3, 1.3−0.8 | 75 |
| NGC 3293 | 6.9−2.2, 2.2−1.2, 1.2−0.8 | 77 |
| NGC 3324 | 6.9−2.1, 2.1−1.2, 1.2−0.8 | 70 |
| Object . | Mass range . | Confidence level . |
|---|---|---|
| . | (M⊙) . | (percentage) . |
| NGC 5617 | 4.0−2.4, 2.4−1.2, 1.2−0.8 | 88 |
| Trumpler 22 | 4.1−2.6, 2.6−1.3, 1.3−0.8 | 75 |
| NGC 3293 | 6.9−2.2, 2.2−1.2, 1.2−0.8 | 77 |
| NGC 3324 | 6.9−2.1, 2.1−1.2, 1.2−0.8 | 70 |
Distribution of stars in different mass ranges along with the percentage of confidence level in the mass-segregation effect for the clusters.
| Object . | Mass range . | Confidence level . |
|---|---|---|
| . | (M⊙) . | (percentage) . |
| NGC 5617 | 4.0−2.4, 2.4−1.2, 1.2−0.8 | 88 |
| Trumpler 22 | 4.1−2.6, 2.6−1.3, 1.3−0.8 | 75 |
| NGC 3293 | 6.9−2.2, 2.2−1.2, 1.2−0.8 | 77 |
| NGC 3324 | 6.9−2.1, 2.1−1.2, 1.2−0.8 | 70 |
| Object . | Mass range . | Confidence level . |
|---|---|---|
| . | (M⊙) . | (percentage) . |
| NGC 5617 | 4.0−2.4, 2.4−1.2, 1.2−0.8 | 88 |
| Trumpler 22 | 4.1−2.6, 2.6−1.3, 1.3−0.8 | 75 |
| NGC 3293 | 6.9−2.2, 2.2−1.2, 1.2−0.8 | 77 |
| NGC 3324 | 6.9−2.1, 2.1−1.2, 1.2−0.8 | 70 |
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.
