Relativistic Theoretical Calculation of O III: Radiative Transition Rates and the Bowen Mechanism in Planetary Nebulae
TONG Xiaomin, ZOU Yu, LI Jiaming, LIU Xiaowei
Institute of Physics, Academia Sinica, Beijing 100080
Department of Physics and Astronomy, University College London, UK
Relativistic Theoretical Calculation of O III: Radiative Transition Rates and the Bowen Mechanism in Planetary Nebulae
TONG Xiaomin;ZOU Yu;LI Jiaming;LIU Xiaowei
Institute of Physics, Academia Sinica, Beijing 100080
Department of Physics and Astronomy, University College London, UK
关键词 ：
31.20.Tz ,
32.70.Cs
Abstract ： A full relativistic configuration interaction (RCI) calculation of transition energies and radiative transition rates involved in O III Bowen fluorescence mechanism is presented. The calculated ratios of transition line intensities are in good agreement with the observed ratios. The discrepancies between the RCI calculation and prediction based on LS coupling scheme show that a delicate balance between the electron correlations and the spin-orbital interactions should be important even for the low-Z O III ion.
Key words ：
31.20.Tz
32.70.Cs
出版日期: 1994-02-01
引用本文:
TONG Xiaomin;ZOU Yu;LI Jiaming;LIU Xiaowei. Relativistic Theoretical Calculation of O III: Radiative Transition Rates and the Bowen Mechanism in Planetary Nebulae
[J]. 中国物理快报, 1994, 11(2): 69-72.
链接本文:
https://cpl.iphy.ac.cn/CN/
或
https://cpl.iphy.ac.cn/CN/Y1994/V11/I2/69
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