Mass segregation effects in very young open clusters
2007 ◽
Vol 3
(S248)
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pp. 481-483
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AbstractWe 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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2004 ◽
Vol 221
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pp. 237-246
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1998 ◽
Vol 188
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pp. 13-16
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2016 ◽
Vol 11
(S321)
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pp. 214-216
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2010 ◽
Vol 6
(S270)
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pp. 103-106
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2019 ◽
Vol 488
(2)
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pp. 2800-2824
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2004 ◽
Vol 202
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pp. 362-364
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2020 ◽
Vol 499
(1)
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pp. 334-354