论文标题
苔丝观察到的原型星$γ$ doradus
The prototype star $γ$ Doradus observed by TESS
论文作者
论文摘要
$γ$ doradus是同名脉动恒星类别的原型恒星，由晚期的a- f次序列恒星组成，以低频重力惯性模式振荡。作为同类恒星中最亮的恒星之一（v = 4.2），$γ$ dor受益于大量观察数据，这些数据最近通过TESS Mission从高质量的空间光度法完成。有了这些新数据，我们建议研究$γ$ dor，作为多技术基础和基于太空观测之间协同作用的可能性的一个例子。在这里，我们介绍了调查的初步结果。
$γ$ Doradus is the prototype star for the eponymous class of pulsating stars that consists of late A-early F main-sequence stars oscillating in low-frequency gravito-inertial modes. Being among the brightest stars of its kind (V = 4.2), $γ$ Dor benefits from a large set of observational data that has been recently completed by high-quality space photometry from the TESS mission. With these new data, we propose to study $γ$ Dor as an example of possibilities offered by synergies between multi-technical ground and space-based observations. Here, we present the preliminary results of our investigations.
