Halo mass of three-dimension milky way
文献类型：期刊论文
| 作者 | Peng Fang2; Peng Qiuhe1 |
| 刊名 | Chinese Physics Letters
 |
| 出版日期 | 2000 |
| 卷号 | 17期号:5页码:385 |
| ISSN号 | 0256-307X |
| 英文摘要 | We emphasize the effects of several factors on halo mass for our Galaxy, such as the disk thickness, the local surface density, and the shape of the rotation curve. By fitting the observed rotation curve of our Galaxy with the five-component model, we deduce a halo with a mass of 6.62x10(11)M(circle dot) within 50 kpc and a local density of 0.009M(circle dot)pc(-3). It is found that the realistic Galaxy needs only about half of the halo mass that the Galaxy with an infinitesmally thin disk requires. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/46893]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.南京大学-中国科学院-北京大学联合天体物理中心 2.南京大学 |
| 推荐引用方式 GB/T 7714 | Peng Fang,Peng Qiuhe. Halo mass of three-dimension milky way[J]. Chinese Physics Letters,2000,17(5):385. |
| APA | Peng Fang,&Peng Qiuhe.(2000).Halo mass of three-dimension milky way.Chinese Physics Letters,17(5),385. |
| MLA | Peng Fang,et al."Halo mass of three-dimension milky way".Chinese Physics Letters 17.5(2000):385. |
入库方式： OAI收割
来源：国家天文台
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