The chemical classification of the AGB star IRAS 17515-2407
文献类型：期刊论文
| 作者 | Chen PS(陈培生)1 ; Zhang P(张品)1,2
|
| 刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2003-12 |
| 卷号 | 3期号:6页码:551-554 |
| 关键词 | stars : AGB stars : chemical classification stars : maser infrared : stars |
| ISSN号 | 1009-9271 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Chen, PS (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | The chemical classification of IRAS 17515-2407 has been debated for a long time. Up to now there are two contenders, oxygen-rich or carbon-rich. We believe that IRAS 17515-2407 is an oxygen-rich source: because (i) it shows the silicate self-absorbed emission; (ii) in the near infrared-IRAS diagram it is located in the oxygen-rich object region and (iii) particularly, it has detected SiO maser emission. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 分类号 | P148 |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | INFRARED CARBON STARS ; LOW-RESOLUTION SPECTROMETER ; POINT-SOURCE CATALOG ; GIANT BRANCH STARS ; NEAR-IR PHOTOMETRY ; CIRCUMSTELLAR ENVELOPES ; SPACE DISTRIBUTION ; DUST SHELLS ; SPECTRA ; EVOLUTION |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1009-9271/3/6/551/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000187404500009 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/4151]  |
| 专题 | 云南天文台_其他 |
| 作者单位 | 1.National Astronomical Observatories, Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 2.Cosmic Ray Institute, Yunnan University, Kunming 650091 |
| 推荐引用方式 GB/T 7714 | Chen PS,Zhang P. The chemical classification of the AGB star IRAS 17515-2407[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2003,3(6):551-554. |
| APA | Chen PS,&Zhang P.(2003).The chemical classification of the AGB star IRAS 17515-2407.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,3(6),551-554. |
| MLA | Chen PS,et al."The chemical classification of the AGB star IRAS 17515-2407".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 3.6(2003):551-554. |
入库方式： OAI收割
来源：云南天文台
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