The Many Routes to AGN Feedback

Frontiers in Astronomy and Space Sciences

Morganti, Raffaella¹ 

[1] ASTRON, Netherlands Institute for Radio Astronomy, Netherlands

关键词: active galactic nuclei;    Interstellar Medium;    Outflows;    extragalactic radio jets;    spectroscopy;   

DOI  :  10.3389/fspas.2017.00042

学科分类：空间科学

来源: Frontiers

【 摘 要 】

The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds or radio plasma jets, is known to impact on the surrounding interstellar medium. The result of these processes, known as AGN (negative) feedback, is suggested to prevent gas, in and around galaxies, from cooling, and to remove, or at least redistribute, gas by driving massive and fast outflows, hence playing a key role in galaxy evolution. Given its importance, a large effort is devoted by the astronomical community to trace the effects of AGN on the surrounding gaseous medium and to quantify their impact for different types of AGN. This review briefly summarizes some of the recent observational results obtained in different wavebands, tracing different phases of the gas. I also summarise new insights they have brought, and the constraints they provide to numerical simulations of galaxy formation and evolution. The recent addition of deep observations of cold gas and, in particular, of cold molecular gas, has brought some interesting surprises and has expanded our understanding of AGN and AGN feedback.

【 授权许可】

CC BY