The local interstellar medium

被引：33

作者：

Ferlet, R ^{[1
]}

机构：

[1] CNRS, Inst Astrophys, F-75014 Paris, France

来源：

ASTRONOMY AND ASTROPHYSICS REVIEW | 1999年 / 9卷 / 3-4期

关键词：

galaxy (the): solar neighbourhood; interstellar medium : clouds : individual : the Local Cloud; interstellar medium : bubbles; interstellar medium : kinematics; interplanetary medium;

D O I：

10.1007/s001590050016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Substantial progress in the field of the Local Interstellar Medium has been largely due to recent launches of space missions, mostly in the UV and X-ray domains, but also to ground-based observations, mainly in high resolution spectroscopy. However, a clear gap seems to remain between the wealth of new data and the theoretical understanding. This paper gives an overview of some observational aspects, with no attempt of completeness or doing justice to all the people involved in the field. As progress rarely evolves in straight paths, we can expect that our present picture of the solar system surroundings is not definitive.

引用

页码：153 / 169

页数：17

共 77 条

[1]

[Anonymous], 1981, Galactic astronomy: Structure and kinematics

[2] THE INFLUENCE OF THE INTERFACE BETWEEN THE HELIOSPHERE AND THE LOCAL INTERSTELLAR-MEDIUM ON THE PENETRATION OF THE H-ATOMS TO THE SOLAR-SYSTEM [J].