Abstract
We derived proper motions and membership probabilities of stars in the regions of two very young (~2 - 4 Myr-old) open clusters NGC 2244 and NGC 6530. Both clusters show clear evidence of mass segregation, which provides strong support for the suggestion that the observed mass segregation is - at least partially - due to the way in which star formation has proceeded in these complex star-forming regions ("primordial" mass segregation).
| Original language | English |
|---|---|
| Pages (from-to) | 481-483 |
| Number of pages | 3 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 3 |
| Issue number | S248 |
| DOIs | |
| Publication status | Published - Oct 2007 |
| Externally published | Yes |
Keywords
- open clusters and associations: general
- open clusters and associations: individual (NGC2244)
- open clusters and associations: individual (NGC6530)