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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.
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页码:276 / 280
页数:5
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