杰克·希尔斯
| 杰克·希尔斯 | |
|---|---|
 杰克·希尔斯 |
杰克·希尔斯（Jack G. Hills）是一名美国天文学家。他曾提出内奥尔特云的概念，该区域因此也冠上他的姓，称为“希尔斯云”[1][2]。他大部分职业生涯都是在美国洛斯阿拉莫斯国家实验室渡过的。从1998年开始，他成为该实验室的研究员[3]。
参考资料[编辑]
- ^ Stellar Dynamics: Jack Hills. Department of Physics and Astronomy. （原始内容存档于15 December 2014）.
- ^ Michael Moltenbrey. Dawn of Small Worlds: Dwarf Planets, Asteroids, Comets. Springer. 24 October 2015: 97 [2019-01-13]. ISBN 978-3-319-23003-0. （原始内容存档于2019-05-13）.
- ^ Laboratory Fellows from 1981 to the present （页面存档备份，存于互联网档案馆） Los Alamos National Security J. G. Hills has made large contributions to Laboratory and international programs in astrophysics, interplanet science, and asteroid interdiction. He also is recognized worldwide as one of the major authorities in the field of stellar dynamics and has made seminal contributions to the quantitative understanding of interactions between binary and single stars in clusters.
拓展阅读[编辑]
- Jack G. Hills. Comet showers and the steady-state infall of comets from the Oort Cloud. Astronomical Journal. 1981, 86: 1730–1740. Bibcode:1981AJ.....86.1730H. doi:10.1086/113058.
- J. G. Hills. Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit. Nature. 1984, 311 (5987): 636–638. Bibcode:1984Natur.311..636H. doi:10.1038/311636a0.
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