The kinematics of the planetary nebula BD+30°3639

被引：21
作者：
Bryce, M
Mellema, G
机构：
[1] Univ Manchester, Dept Phys & Astron, Manchester M13 9PL, Lancs, England
[2] Stockholm Observ, SE-13336 Saltsjobaden, Sweden
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1999年 / 309卷 / 03期
关键词：
ISM : kinematics and dynamics; planetary nebulae : individual : BD+30 degrees 3639;
D O I：
10.1046/j.1365-8711.1999.02892.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we describe the results of the first optical kinematic study of the planetary nebula BD+30 degrees 3639, This system has a central star of the Wolf-Rayet type and is believed to be fairly young. Emission-line spectra were obtained at high spectral and spatial resolution using the Utrecht echelle spectrometer at the William Herschel Telescope. These spectra indicate that the main ionized shell of BD + 30 degrees 3639 appears to be evolving in a more complex way than previously thought.
引用
收藏
页码：731 / 738
页数：8
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