A new, evolved bipolar planetary nebula

被引:0
|
作者
Corradi, RLM [1 ]
Villaver, E [1 ]
Mampaso, A [1 ]
Perinotto, M [1 ]
机构
[1] UNIV FLORENCE, DIPARTIMENTO ASTRON & SCI SPAZIO, I-50125 FLORENCE, ITALY
关键词
planetary nebulae; PN G321.6+02.2;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Optical imaging and spectroscopy reveal that the ionised region No.252 in the list of Marsalkowa (1974), whose photograph is presented in the ''Atlas of Galactic Nebulae'' by Neckel & Vehrenberg (1990), is actually a planetary nebula. According to Acker et al. (1992), the object should therefore be named as PN G321.6+02.2. The nebula has the following properties: it is located at 2.0+/-0.5 kpc from the Sun, has a bipolar morphology, a giant size (similar to 4 pc!), low densities, a hot (unobserved) central star (T>130000 K), and extreme He and N overabundances (He/H=0.147+/-10.029, log(N/O)=0.47(-0.38)(+0.20)). The nebula is likely to be in a very evolved evolutionary stage.
引用
收藏
页码:276 / 280
页数:5
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