| 三个大角径的宇宙γ射线源 |
| |
| 引用本文： | 李惕碚.三个大角径的宇宙γ射线源[J].空间科学学报,1984,4(1):72-75. |
| |
| 作者姓名： | 李惕碚 |
| |
| 作者单位： | 中国科学院高能物理研究所 |
| |
| 摘 要： | 由γ天文卫星COS-B的观测数据及最近的射电天文观测结果的分析表明,2CG036+01、2CG218-00和2CG235-01这三个宇宙γ射线源,可能是一个分子云或沿视线方向若干分子云的迭加形成.
|
| 收稿时间： | 1900-01-01 |
Three Gamma-ray Sources With Large Angular Sizes |
| |
| Institution: | Institute of High Energy Physics, Academia Sinica |
| |
| Abstract: | Based on an analysis of the data from the gamma-ray astronomy satellite COS-Band the radio-astronomy measurements for CO molecules, it appears that the three cosmic gamma-ray sourcer, 2CG 036+01, 2CG 218-00 and 2CG 235-01, should possibly be isolated giant molecular clouds or combinations of some molecular clouds which are aligned within the angular resolution of detector. |
| |
| Keywords: | |
| 本文献已被 CNKI 等数据库收录！ |
| 点击此处可从《空间科学学报》浏览原始摘要信息 |
| 点击此处可从《空间科学学报》下载免费的PDF全文 |
|
