The binary fractions in the massive young Large Magellanic Cloud star clusters NGC 1805 and NGC 1818
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The exclusion of a significant range of ages in a massive star cluster.Gamma-Ray Burst ProgenitorsFormation of new stellar populations from gas accreted by massive young star clustersThe tight subgiant branch of the intermediate-age star cluster NGC 411 implies a single-aged stellar populationThe dynamical importance of binary systems in young massive star clusters
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The binary fractions in the massive young Large Magellanic Cloud star clusters NGC 1805 and NGC 1818
description
im September 2013 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована у вересні 2013
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name
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@en
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@nl
type
label
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@en
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@nl
prefLabel
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@en
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@nl
P2860
P356
P1476
The binary fractions in the ma ...... clusters NGC 1805 and NGC 1818
@en
P2093
Licai Deng
P2860
P304
P356
10.1093/MNRAS/STT1669
P407
P577
2013-09-25T00:00:00Z
P5875
P818
P819
2013MNRAS.436.1497L