Extreme properties of a compact and massive accreting black hole host in the first 500 Myr
Roberta Tripodi, Nicholas S. Martis, Vladan Markov, Maruša Bradač, Fabio Di Mascia, Vieri Cammelli, Francesco D’Eugenio, Chris J. Willott, Mirko Curti, Maulik Bhatt, S. Gallerani, Gregor Rihtaršič, Jasbir Singh, Gaia Gaspar, Anishya Harshan, Jon Judež, Rosa M. Mérida, G. Desprez, Marcin Sawicki, Ilias Goovaerts, Adam Muzzin, Gaël Noirot, Ghassan T. E. Sarrouh, Roberto Abraham, Yoshihisa Asada, Gabriel Brammer, Vicente Estrada-Carpenter, Giordano Felicioni, Seiji Fujimoto, Kartheik G. Iyer, Lamiya Mowla, Victoria Strait
Abstract
relations, suggesting an early, rapid black hole growth preceding that of its galaxy. CANUCS-LRD-z8.6 may represent an evolutionary link between early massive black holes and the luminous quasars observed at z = 6.
Topics & Concepts
PhysicsAstrophysicsActive galactic nucleusRedshiftBlack hole (networking)GalaxyQuasarMetallicityAstronomyGalaxy formation and evolutionBinary black holemyrStellar black holeIntermediate-mass black holeSupermassive black holeCosmologyHost (biology)Spectral lineAstrophysical Phenomena and ObservationsGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical Research