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 |
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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)