Super-Eddington accretion in high-redshift quasar hosts: black-hole driven outflows, galaxy quenching, and the nature of Little Red Dots
BibTeX Entry
@article{2025arXiv250505556Q,
author = {{Quadri}, Giada and {Trinca}, Alessandro and {Lupi}, Alessandro and {Colpi}, Monica and {Volonteri}, Marta},
title = {{Super-Eddington accretion in high-redshift quasar hosts: black-hole driven outflows, galaxy quenching, and the nature of Little Red Dots}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics},
year = {2025},
month = may,
eid = {arXiv:2505.05556},
pages = {arXiv:2505.05556},
archiveprefix = {arXiv},
eprint = {2505.05556},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250505556Q},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, early universe, host galaxy, jwst, simulation},
month_numeric = {5}
}
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