特殊恒星
- 网络peculiar star
特殊恒星-
应用p-ω发电机模型，对一类特殊恒星（CP星）的磁场产生机制进行讨论。
Using the p ω dynamo model , the magnetic field generation mechanism for kinds of special stellar stars is discussed .
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恒星光谱一般具有明显的吸收线或者吸收带特征，而具有发射线的恒星光谱对应着特殊类型的恒星，如激变变星、HerbigAe/Be等。对这些光谱的后续研究有着重要的意义。
Stellar spectra are characterized by obvious absorption lines or absorption bands , while those with emission lines are usually special stars such as Cataclysmic Variable stars ( CVs ), HerbigAe / Be etc. The further study of this kind of spectra is meaningful .