GALACTIC FOUNTAINS

被引:6
作者
KAHN, FD
机构
[1] Department of Astronomy, The University, Manchester
关键词
D O I
10.1007/BF00982513
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The hot intercloud medium (ICM) streams away from the Galactic disk into the fountain. It is generally agreed that a flow consisting of thermal gas only reaches a maximum height of a few (3 to 5) kpc. The dynamics is more complicated if cosmic rays are also present. In that case it is possible for some of the gas to be ejected from the Galaxy altogether.
引用
收藏
页码:325 / 332
页数:8
相关论文
共 14 条
[1]  
Bloemen, 1991, IAU S, V144
[2]   THE GALACTIC FOUNTAIN OF HIGH-VELOCITY CLOUDS [J].
BREGMAN, JN .
ASTROPHYSICAL JOURNAL, 1980, 236 (02) :577-591
[3]  
BREITSCHWERDT D, 1993, ASTRON ASTROPHYS, V269, P54
[4]  
HEILES C, 1989, IAU C, V120, P484
[5]  
Kahn F. D., 1981, Investigating the universe, P1
[6]  
KAHN FD, 1976, ASTRON ASTROPHYS, V50, P145
[7]   MAGNETIC RECONNECTION IN THE DISC AND HALO [J].
KAHN, FD ;
BRETT, L .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1993, 263 (01) :37-48
[8]  
KAHN FD, 1991, IAU S, V144, P1
[9]   THE GIANT AND SUPER-GIANT SHELLS OF THE MAGELLANIC CLOUDS [J].
MEABURN, J .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1980, 192 (02) :365-&
[10]  
MULLER CA, 1963, CR HEBD ACAD SCI, V257, P1661