NAOC Open IR
晚型星计算机自动光谱分类
李金增; 胡景耀
1999
Source Publication天体物理学报
ISSN0253-2379
Volume019Issue:003Pages:297
Abstract在对恒星形成区(SFR)中ROSAT选弱发射线T Tauri星(WTTS)进行光谱证认的过程中,发展了一套基于北京天文台2.16米光学望远镜及其OMR卡焦光谱仪系统的晚型星中色散(50A/mm)光谱计算机自动光谱分类方法。对ROSAT选WTTS候选体中晚型星进行自动光谱分类的结果表明,一般情况下,光谱型的分类精度可达±1个次级,个别源为±2个次级。该自动光谱分类方法同时适用于其它光谱晚型星。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/43916
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
李金增,胡景耀. 晚型星计算机自动光谱分类[J]. 天体物理学报,1999,019(003):297.
APA 李金增,&胡景耀.(1999).晚型星计算机自动光谱分类.天体物理学报,019(003),297.
MLA 李金增,et al."晚型星计算机自动光谱分类".天体物理学报 019.003(1999):297.
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