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
{{i.achievement_title}}
数据更新时间:2023-05-31
Mechanism of allosteric activation of SIRT6 revealed by the action of rationally designed activators
Molecular dynamics simulations on evaporation of a suspended binary mixture nanodroplet
Tuning the subsurface oxygen of Ag2O-derived Ag nanoparticles to achieve efficient CO2 electroreduction to CO
Spin dynamics characteristics of nitrogen vacancy spins in diamond films using enhanced Raman shift with spin microscopy
Organic geochemical characteristics and accumulation of the organic matterin the Jurassic to Cretaceous sediments of the Saihantala Sag, Erlian Basin,China
星系中球状星团的形成机制预研究
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
漩涡星系的基本面