Simulations on Radio Galaxies with Magnetic Tower Model--Indications for Jet Feedback

来源 :Black Hole Accretion and AGN Feedback(黑洞的吸积和AGN反馈学术会议) | 被引量 : 0次 | 上传用户：bcdagjcly

【摘要】

：

Jets are powerful,collimated and Large-scale The power of jets is usually sufficient enough to bias the galaxy evolution(e.g.,to quench cooling flow),but How does jet energy dissipate into ISM/ICM/IGM

【作者】

：

Zhaoming Gan Hui Li Shengtai Li Feng Yuan

【机构】

：

SHAO LANL

【出处】

：

Black Hole Accretion and AGN Feedback(黑洞的吸积和AGN反馈学术会议)

【发表日期】

：

2015年5期

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Simulations on Radio Galaxies with Magnetic Tower Model--Indications for Jet Feedback

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