Dynamic stars: atmospheres, evolution and asteroseismology

通过发展最先进的恒星大气和演化模型，该项目将努力回答恒星天体物理学中的一些关键问题，包括磁场如何在恒星中表现出来，恒星如何受到对流的影响，恒星如何激发振荡以及银河系中最古老的恒星有多老。该项目将努力淘汰过去半个世纪以来阻碍恒星建模的自由参数。利用独特的恒星模型，该项目旨在为现代天文学的无数研究提供丰富的遗产资源，并为雄心勃勃的澳大利亚领导的银河系调查提供必要的理论基础，如GALAH和SkyMapper，以及国际卫星任务，如开普勒、苔丝和柏拉图。

By developing state-of-the-art stellar atmosphere and evolution models, the project will endeavour to answer some of the key outstanding questions in stellar astrophysics including how magnetic fields are manifested in stars, how stars are affected by convection, how oscillations are excited in stars and how old the most ancient stars in the Milky Way are. The project will endeavour to make obsolete the free parameters that have hampered stellar modelling for the past half-century. Using unique stellar models the project aims to provide rich legacy resources for countless studies in modern astronomy and provide the necessary theoretical underpinning for ambitious Australian-led Milky Way surveys, such as GALAH and SkyMapper, and international satellite missions such as Kepler, TESS and PLATO.