Using a combined observational and numerical approach I propose to address two questions with far-reaching consequences for fields ranging from star and cluster formation to galaxy formation and evolution: What are the initial (dynamical and environmental) conditions and star-formation efficiencies required for star cluster formation? and What fraction of star clusters can survive to old age
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数据更新时间:2023-05-31
Achieving secure communications in multi-antenna cooperative cognitive radio networks using cooperative jamming
The fracture behavior of twinned Cu nanowires: Amolecular dynamics simulation
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Robust adaptive control of uncertain nonlinear systems with unmodeled dynamics using command filter
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银河系疏散星团的基本参数与银河系结构
等级成团星系形成机制下球状星团的形成演化
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