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Título: | Multi-Wavelength and Multi-Messenger Studies Using the Next-Generation Event Horizon Telescope |
Autor: | Lico, Rocco; Jorstad, Svetlana G.; Marscher, Alan P.; Gómez, José L. CSIC ORCID ; Liodakis, Ioannis; Dahale, Rohan; Alberdi, Antxón CSIC ORCID ; Gold, Roman; Traianou, E.; Toscano, Teresa; Foschi, Marianna | Palabras clave: | Very long baseline interferometry (VLBI) Supermassive black holes Active galactic nuclei Multi-wavelength studies Relativistic jets |
Fecha de publicación: | 14-ene-2023 | Editor: | Multidisciplinary Digital Publishing Institute | Citación: | Galaxies 11(1): 17 (2023) | Resumen: | 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. © 2023 by the authors. Licensee MDPI, Basel, Switzerland. | Descripción: | This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). | Versión del editor: | http://dx.doi.org/10.3390/galaxies11010017 | URI: | http://hdl.handle.net/10261/309475 | DOI: | 10.3390/galaxies11010017 | E-ISSN: | 2075-4434 |
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2023Galax..11...17L.pdf | 4,52 MB | Adobe PDF | Visualizar/Abrir |
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