Eclipsing binaries and related photometry

Yitang Chen
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Abstract

This work mainly focuses on eclipsing binaries. It classifies binary stars based on the way they are discovered and chooses eclipsing binaries as the major topic. Firstly, the paper defines that the criteria for classifying eclipsing binaries in this work are Roche lobe by conductions, which divides eclipsing binaries into three kinds. To further explore the characteristics of three different types of eclipsing binaries, this paper applies light curve analysis, an extremely useful method for finding and analyzing binaries on them, and conducts some special features. Based on the analysis, this paper connects the conduction of the Roche lobe with observation data together. Nowadays, research on binary stars is prevalent because they are related to discovering exoplanets. Research on binary stars contributes to the development of discovering exoplanets as well. A couple of methods in finding binary stars can be applied in finding exoplanets, which have dramatic practical utilizations.
食双星和相关测光
这项工作主要关注食双星。它根据发现双星的方式对双星进行分类,并选择食双星作为主要课题。首先,论文定义了本文中的食双星分类标准是罗切叶导,将食双星分为三种。为了进一步探究三种不同类型的食双星的特征,本文应用了光曲线分析这种对发现和分析食双星非常有用的方法,并对一些特殊的特征进行了分析。在分析的基础上,本文将罗氏叶的传导与观测数据联系在一起。如今,对双星的研究非常普遍,因为它们与发现系外行星有关。对双星的研究也有助于系外行星的发现。寻找双星的几种方法可以应用于寻找系外行星,这些方法具有巨大的实际用途。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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