Production of 2H, 3He, and 7Li from interactions between jets and clouds

被引:3
作者
Famiano, M
Vandegriff, J
Boyd, RN
Kajino, T
Osmer, P
机构
[1] Ohio State Univ, Dept Phys, Smith Lab, Columbus, OH 43210 USA
[2] Ohio State Univ, Dept Astron, McPherson Lab, Columbus, OH 43210 USA
[3] Natl Astron Observ, Tokyo 1818588, Japan
[4] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[5] Grad Univ Adv Studies, Dept Astron Sci, Tokyo 1818588, Japan
基金
美国国家科学基金会;
关键词
galaxies : jets; nuclear reactions; nucleosynthesis; abundances;
D O I
10.1086/318879
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The interactions between jets of high-energy nuclei and nuclei of the surrounding medium are studied. Such interactions could be initiated by jets from active galactic nuclei interacting with surrounding cool clouds. The resulting nuclear interactions are found to produce copious amounts of H-2 and He-3 from the He-4 nuclei. These results suggest that jets of particles from quasars could have produced anomalously high abundances in surrounding clouds of some of the nuclides usually thought to characterize big bang nucleosynthesis, specifically, the H-2 seen in absorption spectra.
引用
收藏
页码:L21 / L24
页数:4
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