Three dimensional resolution of the strongly magnetic photospheres and upper atmospheres of the rapidly oscillating peculiar A stars

快速振荡的奇特 A 星的强磁光球层和高层大气的三维分辨率

• 批准号: ST/F002203/1
• 负责人: Donald Kurtz
• 金额: $ 30.72万
• 依托单位: University of Central Lancashire
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2008
• 资助国家: 英国
• 起止时间: 2008 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FF002203%2F1
• 关键词: Three; dimensional; resolution; strongly; magnetic

Asteroseismology uses sounds in stars to probe their interiors. Just as ultrasound is used to see the face of a foetus before it is born, astronomers can 'see' inside the stars by studying their light variations caused by pulsations within them. This research will provide unprecedent 3D views of the pulsation modes and abundance distributions in the rapidly oscillating peculiar A stars.

星震学利用恒星的声音来探测其内部。就像超声波被用来在胎儿出生前看到胎儿的脸一样，天文学家可以通过研究恒星内部脉动引起的光线变化来“看到”恒星内部。这项研究将为快速振荡的特殊A星的脉动模式和丰度分布提供前所未有的三维视图。