NAOC Open IR
iras172133841晚型富碳星还是早型发射线星
陈培生; 张品
2003
Source Publication天文学报
ISSN0001-5245
Volume044Issue:004Pages:350
AbstractIRAS 17213-3841作为富碳星列于新版碳星星表中.然而该星的IRAS低分辨率光谱显示富氧的硅酸盐发射特征;光谱观测结果表明,该星是一个接近零龄主序的,光谱型为O9/B0的早型发射线星,而不是碳星,因此应从碳星星表中剔除.此外,将它证认为碳星的近红外-IRAS双色图方法并不是一个完全可靠的方法,用这一方法来证认碳星必须十分小心.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47645
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
陈培生,张品. iras172133841晚型富碳星还是早型发射线星[J]. 天文学报,2003,044(004):350.
APA 陈培生,&张品.(2003).iras172133841晚型富碳星还是早型发射线星.天文学报,044(004),350.
MLA 陈培生,et al."iras172133841晚型富碳星还是早型发射线星".天文学报 044.004(2003):350.
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