Mass segregation effects in very young open clusters

Details Mass segregation effects in very young open clusters Mass segregation effects in very young open clusters

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..248..481c&link_type=abstract

A Giant Step: from Milli- to Micro-arcsecond Astrometry, Proceedings of the International Astronomical Union, IAU Symposium, Vol

Astronomy and Astrophysics

Astronomy

Open Clusters And Associations: General, Open Clusters And Associations: Individual (Ngc2244), Open Clusters And Associations: Individual (Ngc6530)

Scientific paper

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).

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