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AGB星红外谱的辐射模型及其拟合方法
引用本文:熊关柱,陈建宝.AGB星红外谱的辐射模型及其拟合方法[J].天文学报,1994,35(1):20-26.
作者姓名:熊关柱  陈建宝
作者单位:中国科学院光学天文联合实验室,中国科学院云南天文台,云南大学统计系
摘    要:本文讨论了有拱星壳层的AGB星的红外辐射的双黑体模型并给出了便于似合某些AGB星的红外辐射的双黑体模型并给出了便于拟合某些AGB星的红外观测数据的数学表达式,应用Taylor级数方法解决了这一复杂非线性模型拟合的困难,从而得出了一些AGB星较合理的中心星及壳层的色温度和红外能谱曲线。

关 键 词:AGB星  红外光谱  辐射模型  拟合

THE RADIATION MODEL AND ITS FITTING METHOD FOR THE INFRARED SPECTRUM OF AGB STARS
Xiong Guan-zhu, Chen Pei-sheng.THE RADIATION MODEL AND ITS FITTING METHOD FOR THE INFRARED SPECTRUM OF AGB STARS[J].Acta Astronomica Sinica,1994,35(1):20-26.
Authors:Xiong Guan-zhu  Chen Pei-sheng
Abstract:It is important and difficult for the fitting of the infrared spectrum of AGB stars. This is of vital importance to the determination of many physical parameters. In this paper, the double-blackbody model for the infrared spectrum of AGB stars is built, and by using Taylor series method, the difficulty of this complex non-linear model fitting is solved. Taking this fitting method, we get the more accurate color temperatures of the central stars and dust shells of AGB stars, and the more reasonable infrared spectruni curves.
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