Multi-Wavelength and Multi-Messenger Studies Using the Next-Generation Event Horizon Telescope

被引:5
|
作者
Lico, Rocco [1 ,2 ]
Jorstad, Svetlana G. [3 ,4 ]
Marscher, Alan P. [3 ]
Gomez, Jose L. [1 ]
Liodakis, Ioannis [5 ]
Dahale, Rohan [1 ]
Alberdi, Antxon [1 ]
Gold, Roman [6 ]
Traianou, Efthalia [1 ]
Toscano, Teresa [1 ]
Foschi, Marianna [1 ]
机构
[1] CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, Granada 18008, Spain
[2] INAF Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy
[3] Boston Univ, Inst Astrophys Res, 725 Commonwealth Ave, Boston, MA 02215 USA
[4] St Petersburg State Univ, Astron Inst, Univ Skij Pr 28, St Petersburg 198504, Russia
[5] Univ Turku, Finnish Ctr Astron ESO, FI-20014 Turku, Finland
[6] Univ Southern Denmark, CP3 Origins, Campusvej 55, DK-5230 Odense, Denmark
来源
GALAXIES | 2023年 / 11卷 / 01期
关键词
very long baseline interferometry (VLBI); supermassive black holes; active galactic nuclei; multi-wavelength studies; relativistic jets; ACTIVE GALACTIC NUCLEUS; BLACK-HOLE; JET; ENERGY;
D O I
10.3390/galaxies11010017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The next-generation Event Horizon Telescope (ngEHT) will provide us with the best opportunity to investigate supermassive black holes (SMBHs) at the highest possible resolution and sensitivity. With respect to the existing Event Horizon Telescope (EHT) array, the ngEHT will provide increased sensitivity and uv-coverage (with the addition of new stations), wider frequency coverage (from 86 GHz to 345 GHz and higher), finer resolution (<15 micro-arcseconds), and better monitoring capabilities. The ngEHT will offer a unique opportunity to deeply investigate the physics around SMBHs, such as the disk-jet connection, the mechanisms responsible for high-energy photon and neutrino events, and the role of magnetic fields in shaping relativistic jets, as well as the nature of binary SMBH systems. In this white paper we describe some ngEHT science cases in the context of multi-wavelength studies and synergies.
引用
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页数:9
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