Disentangling AGN-host galaxy interactions from an X-ray perspective

来源 :国际天文学联合会第312次专题会议 | 被引量 : 0次 | 上传用户:lcm0153
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  The circum-nuclear region in an active galaxies is often complex with presence of high excitation gas,collimated radio outflow,and starburst,besides the actively accreting super massive black hole.In studies of a number of archetypal Seyfert galaxies,we were able to evaluate the impact from the AGN by measuring mass outflow and shock heating by radio jet.For galaxies in the throes of a violent merging event such as NGC6240,we were able to resolve 70 MK hot gas surrounding the binary active black holes and discovered a large scale soft X-ray halo.The unique resolving power of Chandra X-ray imaging also enables more discovery of such dual AGN systems.
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