A NEAR-INFRARED VIEW OF SNR - MOLECULAR CLOUD INTERACTIONS

被引：14
|
作者：
BURTON, M
SPYROMILIO, J
机构：
来源：
PROCEEDINGS ASTRONOMICAL SOCIETY OF AUSTRALIA | 1993年 / 10卷 / 04期
关键词：
D O I：
10.1017/S1323358000025960
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Spectroscopic imaging of the SNR RCW 103 has revealed extensive emission in near-infrared lines of H-2 and [Fe II], where the blast wave is encountering a molecular cloud. The H-2 appears to be located outside the [FeII], a morphology which challenges our understanding of shock wave physics. It is suggested that reverse shocks may be responsible for the phenomenom.
引用
收藏
页码：327 / 330
页数：4
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