Shock structure of the high-velocity water masers in W49 N

被引：0
|
作者：
Liljestrom, T [1 ]
机构：
[1] Helsinki Univ Technol, Metsahovi Radio Res Stn, FIN-02150 Espoo, Finland
来源：
RADIO EMISSION FROM GALACTIC AND EXTRAGALACTIC COMPACT SOURCES | 1998年 / 144卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Magnetic field parameters and other characteristics of the postshocked gas in W49 N are derived from a linewidth comparison between the multi-epoch VLBI data of Gwinn and contemporaneous long-term single-dish observations. The observations support predictions of dissociative shock models.
引用
收藏
页码：251 / 252
页数：2
相关论文
共 50 条
12345