Studies of the ISM in the Vela supernova remnant

被引:1
|
作者
Danks, AC
机构
[1] Raytheon ITSS, Greenbelt, MD 20771 USA
[2] GSFC, Greenbelt, MD 20771 USA
关键词
D O I
10.1023/A:1002607404565
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent observations of the Vela SNR in the ISM species Ca II and Na I are presented and discussed in the context of the "break-down'' of the Spitzer-Routly effect. Variations in line profiles with time are demonstrated, eventually through a statistical approach a description of cloud structure will be possible. The IS lines in similar to 70 sightlines are used to determine an accurate distance to the Vela SNR of 250 +/- 30 pc. Finally a discussion of future observations are given relating information obtained from measurements of near-by ISM to more distant intergalactic medium.
引用
收藏
页码:127 / 133
页数:7
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