系外行星宿主恒星的表征
地球与行星天体物理
2017-11-29 v1 太阳与恒星天体物理
摘要
精确且尽可能准确的系外行星表征无法与其宿主恒星的表征相分离。在本章中，我们讨论用于推导系外行星宿主恒星基本性质和大气参数的不同方法与技术。介绍了每种方法的主要局限、优势与劣势，以及相应的典型测量不确定度。
引用
@article{arxiv.1711.01112,
title = {Characterization of Exoplanet-Host Stars},
author = {Vardan Adibekyan and Sérgio G. Sousa and Nuno C. Santos},
journal= {arXiv preprint arXiv:1711.01112},
year = {2017}
}
备注
Lecture presented at the IVth Azores International Advanced School in Space Sciences on "Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds" (arXiv:1709.00645), which took place in Horta, Azores Islands, Portugal in July 2016