The interstellar environment of our galaxy

被引:802
作者
Ferrière, KM [1 ]
机构
[1] Observ Midi Pyrenees, F-31400 Toulouse, France
关键词
D O I
10.1103/RevModPhys.73.1031
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This article reviews the current knowledge and understanding of the interstellar medium of our galaxy. The author first presents each of the three basic constituents-ordinary matter, cosmic rays, and magnetic fields-of the interstellar medium, with emphasis on their physical and chemical properties as inferred from a broad range of observations. The interaction of these interstellar constituents, both with each other and with stars, is then discussed in the framework of the general galactic ecosystem.
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页码:1031 / 1066
页数:36
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共 351 条
[2]  
ABBOTT DC, 1987, ANNU REV ASTRON ASTR, V25, P113
[4]  
[Anonymous], 1981, Galactic astronomy: Structure and kinematics
[5]  
ASCHENBACH B, 1988, IAU C, V101, P99
[6]   EXTRAGALACTIC MAGNETIC-FIELDS [J].
ASSEO, E ;
SOL, H .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1987, 148 (06) :307-436
[7]  
Axford W. I., 1977, INT COSMIC RAY C, P132
[8]   THE PHOTOELECTRIC HEATING MECHANISM FOR VERY SMALL GRAPHITIC GRAINS AND POLYCYCLIC AROMATIC-HYDROCARBONS [J].
BAKES, ELO ;
TIELENS, AGGM .
ASTROPHYSICAL JOURNAL, 1994, 427 (02) :822-838
[9]  
BARTUNOV OS, 1992, ASTRON ASTROPHYS, V264, P428
[10]  
Beals CS, 1935, MON NOT R ASTRON SOC, V96, P0661