According to the simplified unification model of active galactic nuclei ( AGN), assuming that the gas in the NLR is spherically distributed, V-shape morphology ( ionization cone) is expected to be observed in Seyfert 2 galaxy.

  • 根据简化的活动星系核的统一模型,假设窄线区气体成球状分布,那么应观测到塞弗特2型星系的窄线区电离气体成V状(电离锥)。

  • 互联网摘选 2025-01-20 17:42:11

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