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ELECTRON-IMPACT EXCITATION OF INTERSTELLAR MOLECULES

机译:星际分子的电子冲击激发

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Electron-molecule collisions play a crucial role in as-trophysical environments where the electron fraction is higher than about 10~(-5), e.g. in the diffuse ISM, PDRs or comets. We present here a brief review of our recent R-matrix calculations of rate coefficients for electron-impact excitation of interstellar molecules. Our major result is the prediction of emission lines from higher rotational states than previously assumed. Rate coefficients for transitions with Δj > 1 are indeed found to be significant and in some cases larger than those with Δj = 1, the only ones considered previously. This reflects the importance of short-range interactions which are ignored in the standard theories. Illustrative results are presented for CH~+, H_3~+ and H_2O.
机译:电子分子碰撞在天体环境中起着至关重要的作用,在天体环境中,电子分数高于约10〜(-5),例如在分散的ISM,PDR或彗星中。我们在这里简要回顾一下我们最近的星际分子电子碰撞激发速率系数的R矩阵计算。我们的主要结果是根据比以前假定的更高的旋转状态预测发射线。实际上,发现Δj> 1的跃迁的速率系数非常重要,并且在某些情况下比Δj= 1的跃迁系数更大,这是以前才考虑的。这反映了标准理论中忽略的短程相互作用的重要性。给出了CH〜+,H_3〜+和H_2O的示例性结果。

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