Uncovering the First AGN Jets with AXIS

被引:4
|
作者
Connor, Thomas [1 ]
Banados, Eduardo [2 ]
Cappelluti, Nico [3 ]
Foord, Adi [4 ]
机构
[1] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
[2] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
[3] Univ Miami, Dept Phys, Coral Gables, FL 33124 USA
[4] Univ Maryland Baltimore Cty, Dept Phys, 1000 Hilltop Cir, Baltimore, MD 21250 USA
关键词
active galaxies; X-ray astronomy; supermassive black holes; Advanced X-ray Imaging Satellite; ACTIVE GALACTIC NUCLEI; X-RAY JET; BLACK-HOLES; MULTIWAVELENGTH; MORPHOLOGY; STARS;
D O I
10.3390/universe10050227
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Jets powered by AGN in the early Universe (z greater than or similar to 6) have the potential to not only define the evolutionary trajectories of the first-forming massive galaxies but to enable the accelerated growth of their associated SMBHs. Under typical assumptions, jets could even rectify observed quasars with light seed formation scenarios; however, not only are constraints on the parameters of the first jets lacking, observations of these objects are scarce. Owing to the significant energy density of the CMB at these epochs capable of quenching radio emission, observations will require powerful, high angular resolution X-ray imaging to map and characterize these jets. As such, AXIS will be necessary to understand early SMBH growth and feedback. This White Paper is part of a series commissioned for the AXIS Probe Concept Mission; additional AXIS White Papers can be found at the AXIS website.
引用
收藏
页数:9
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