Super-Eddington accretion in high-redshift quasar hosts: Black-hole-driven outflows, galaxy quenching, and the nature of little red dots

BibTeX Entry

@article{2025A&A...704A.248Q,
  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 = {\aap},
  keywords = {accretion, accretion disks, galaxies: evolution, galaxies: formation, quasars: supermassive black holes},
  year = {2025},
  month = dec,
  volume = {704},
  eid = {A248},
  pages = {A248},
  doi = {10.1051/0004-6361/202555423},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2025A\&A...704A.248Q},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {black hole mass, early universe, host galaxy, jwst, simulation},
  month_numeric = {12}
}

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