Hot haloes of planetary nebulae

被引:0
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作者
Tylenda, R [1 ]
机构
[1] Nicholas Copernicus Astron Ctr, Dept Astrophys, PL-87100 Torun, Poland
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暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present model results of time-dependent ionization of a nebula with a halo. Fast transition of the ionization front across the halo causses its heating well above the equilibrium temperature. For a long time after this event the halo is observed as hotter than the main inner nebula, in agreement with observations of some planetary nebulae.
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页码:451 / 452
页数:2
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