The Chemical Classification of the AGB Star IRAS 17515-2407
文献类型：期刊论文
| 作者 | Chen Peisheng; Zhang Pin |
| 刊名 | Chinese Journal of Astronomy and Astrophysics
 |
| 出版日期 | 2003 |
| 卷号 | 3期号:6页码:551 |
| ISSN号 | 1009-9271 |
| 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. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/39797]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Chen Peisheng,Zhang Pin. The Chemical Classification of the AGB Star IRAS 17515-2407[J]. Chinese Journal of Astronomy and Astrophysics,2003,3(6):551. |
| APA | Chen Peisheng,&Zhang Pin.(2003).The Chemical Classification of the AGB Star IRAS 17515-2407.Chinese Journal of Astronomy and Astrophysics,3(6),551. |
| MLA | Chen Peisheng,et al."The Chemical Classification of the AGB Star IRAS 17515-2407".Chinese Journal of Astronomy and Astrophysics 3.6(2003):551. |
入库方式： OAI收割
来源：国家天文台
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