Investigating the computational and statistical aspects of star and planet formation

年轻的恒星经常在高密度环境中被发现，这意味着年轻恒星之间的相遇可能很常见，这将改变它们的双星性质并影响行星形成盘。博士学位将涉及研究年轻恒星及其环境的各种计算和统计方面。这些包括恒星动力学的动力学和流体动力学模拟，复杂分布的统计措施，检查和解释观测，模拟和“假”数据。

Young stars are often found in high-density environments, this means that encounters between young stars can be common and this will change their binary properties and affect planet-forming discs. A PhD would involve investigating various computational and statistical aspects of young stars and their environments. These include dynamical and hydrodynamical simulations of stellar dynamics, statistical measures of complex distributions, examining and interpreting both observational, simulated and 'fake' data.