AGN的反馈

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Shen（讨论 | 贡献）2024年7月10日 (三) 01:39的版本
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  • 这两篇文章都说Outflow对恒星形成的抑制并不明显[1][2]
  • 射电源的年龄和[OIII]强度相关，反应了反馈的过程（ Our main conclusion is that the [OIII] gas is ∼3 times more likely to be disturbed in the peaked spectrum (PS) sources (that represent a young phase of activity) than non-peaked spectrum (NPS) sources (that represent more evolved sources) at z<0.4. This changes to a factor of ∼2 at z>0.4.）[3]
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