thespatialdistributionofoldneutronstarsinthegalaxy
文献类型：期刊论文
| 作者 | Wei Yingchun2; Zhang Chengmin2 ; Wu Xinji1; Zhao Yongheng2; Chou Chikang2; Luo Ali2
|
| 刊名 | sciencechinaphysicsmechanicsastronomy
 |
| 出版日期 | 2010 |
| 卷号 | 53期号:10页码:1939 |
| ISSN号 | 1674-7348 |
| 英文摘要 | The spatial distributions of old neutron stars (NSs) with ages 10~9 to 10~(10) yr in our Galaxy are investigated by Monte Carlo simulation under two different initial random velocity models. It is found that the scale heights of the distribution increase with the Galactic radial distance. The location of the peak of the NS distribution is closer to the Galactic center than that of their progenitors. The results from our detailed numerical analysis reveal that there is resemblance between the simulated old NS distribution and the structure of the observed HI disk |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/46568]  |
| 专题 | 光学部_LAMOST运行和发展中心 |
| 作者单位 | 1.北京大学 2.中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Wei Yingchun,Zhang Chengmin,Wu Xinji,et al. thespatialdistributionofoldneutronstarsinthegalaxy[J]. sciencechinaphysicsmechanicsastronomy,2010,53(10):1939. |
| APA | Wei Yingchun,Zhang Chengmin,Wu Xinji,Zhao Yongheng,Chou Chikang,&Luo Ali.(2010).thespatialdistributionofoldneutronstarsinthegalaxy.sciencechinaphysicsmechanicsastronomy,53(10),1939. |
| MLA | Wei Yingchun,et al."thespatialdistributionofoldneutronstarsinthegalaxy".sciencechinaphysicsmechanicsastronomy 53.10(2010):1939. |
入库方式： OAI收割
来源：国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。