The kinematics of the planetary nebula BD+30°3639

被引:20
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
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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