NAOC Open IR
irasl92271700富碳星还是富氧星
陈培生; 何金华; 汪洵浩
2003
Source Publication天文学报
ISSN0001-5245
Volume044Issue:001Pages:3
AbstractIRASl9227+1700作为富碳星列于新版碳星星表中.然而该星在IRAS红外双色图上处于典型的有较厚富氧拱星包层区域中,而不处于硅酸盐碳星通常所处的区域.而且有证据表明该星不但有主线和伴线羟基脉泽发射,还有靠近中心星的水脉泽发射.其IRASLRS谱在9—12μm范围有尘埃发射特征,近红外的观测又证实它确实存在热的拱星包层.因此IRAS19227+1700的拱星包层应该全是富氧性质的,它的中心星是富氧的可能性也极大.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37841
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,何金华,汪洵浩. irasl92271700富碳星还是富氧星[J]. 天文学报,2003,044(001):3.
APA 陈培生,何金华,&汪洵浩.(2003).irasl92271700富碳星还是富氧星.天文学报,044(001),3.
MLA 陈培生,et al."irasl92271700富碳星还是富氧星".天文学报 044.001(2003):3.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[陈培生]'s Articles
[何金华]'s Articles
[汪洵浩]'s Articles
Baidu academic
Similar articles in Baidu academic
[陈培生]'s Articles
[何金华]'s Articles
[汪洵浩]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[陈培生]'s Articles
[何金华]'s Articles
[汪洵浩]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.