DIRECT EVIDENCE FOR AN ENERGETIC STELLAR WIND IN NGC-6302

被引：0
|
作者：
MEABURN, J
WALSH, JR
机构：
[1] Department of Astronomy, University of Manchester, Oxford Road, Manchester, United Kingdom
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1980年 / 191卷 / 01期
关键词：
Stellar wind;
D O I：
10.1093/mnras/191.1.5P
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
An 800 km-1 wide wing has been found on profiles of the [Ne v] 3426 Å line from the wind-driven nebula NGC 6302. It is proposed that the emission from a radiatively ionized stellar wind is being observed for the first time. © Royal Astronomical Society.
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页码：P5 / &
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