论文标题
大量OB星的定量光谱指南的现代指南
A modern guide to quantitative spectroscopy of massive OB stars
论文作者
论文摘要
定量光谱是一种强大的技术，我们可以从中提取有关恒星的物理特性和表面化学成分的信息。在本章中，我指导读者了解在学习过程中启动的主要思想，以成为最先进的定量光谱技术在大型OB明星研究中应用专家。 NB：本章旨在为年轻学生服务，作为在过去20年中引起我注意的领域的第一种方法。我应该指出的是，尽管它很重要，但目前，世界各地的真正专家数量仅限于50人，而其中约三分之一的人接近退休。因此，我认为这是一个很好的时刻，写一篇有关该主题的摘要文本，以作为有兴趣加入大型明星船员的下一代学生的指南。如果您是其中之一，请使用本章作为第一个工作笔记本。不要在这里停下来。有关更多详细信息，请挖掘我沿文本引用的文献。而且，一旦到达那里，更深入地挖掘了所有原始资源，以更详细地解释目前已纳入我们现代（几乎）自动化工具中的物理和技术概念。
Quantitative spectroscopy is a powerful technique from which we can extract information about the physical properties and surface chemical composition of stars. In this chapter, I guide the reader through the main ideas required to get initiated in the learning process to become an expert in the application of state-of-the-art quantitative spectroscopic techniques to the study of massive OB stars. NB: This chapter is intended to serve to young students as a first approach to a field which has attracted my attention during the last 20 years. I should note that, despite its importance, at present, the number of real experts in the field around the world is limited to less than 50 people, and about one third of them are close to retirement. Hence, I consider that this is a good moment to write a summary text on the subject to serve as guideline for the next generations of students interested in joining the massive star crew. If you are one of them, please, use this chapter as a first working notebook. Do not stop here. Dig also, for further details, into the literature I quote along the text. And, once there, dig even deeper to find all the original sources explaining in more detail the physical and technical concepts that are presently incorporated into our modern (almost) automatized tools.
