首页> 外文期刊>The Astrophysical Journal. Supplement Series >Accurate ritz wavelengths of parity-forbidden [CoII] and [V II] lines of astrophysical interest
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Accurate ritz wavelengths of parity-forbidden [CoII] and [V II] lines of astrophysical interest

机译:精确的触觉波长的奇偶诊断[COII]和[v II]天体物理兴趣线

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摘要

We report a comprehensive list of accurate Ritz wavelengths for parity-forbidden [Co II] and [V II] lines obtained from the analysis of energy levels measured in the laboratory with Fourier transform emission spectroscopy. Such lines, particularly those in the infrared, are in demand for the analysis of low-density astrophysical plasmas in and around objects such as planetary nebulae, star-forming regions, and active galactic nuclei. Transitions between all known metastable levels of Co II and V II are included in our analysis, producing wavelengths for 1477 [V II] lines and 782 [Co II] lines. Of these, 170 [V II] lines and 171 [Co II] lines arise from transitions with calculated transition probabilities greater than 1 × 10~(-2) s~(-1) and upper level excitations of less than 5 eV, and thus are likely to be observed in astrophysical spectra.
机译:我们报告了额定禁止的近奇的ritz波长的综合列表,并且从具有傅里叶变换发射光谱测量的实验室测量的能量水平分析获得的[v ii]线。 这种线,特别是那些在红外线中,是对诸如行星星云,星形地区和活性半乳核等物体中和周围的低密度天体物理等离子体的分析。 所有已知的亚铁水平的CO II和V II之间的转变包括在我们的分析中,产生1477 [V II]线和782 [CO II]线的波长。 其中,170 [V II]线和171 [CO II]从具有大于1×10〜(-2)S〜(-1)的转换率的转变和少于5eV的上层激发 因此,可能在天体物理学光谱中观察到。

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