The warm outer layer of a little red dot as the source of [Fe II] and collisional Balmer lines with scattering wings

BibTeX Entry

@article{2026A&A...707A..75T,
  author = {{Torralba}, Alberto and {Matthee}, Jorryt and {Pezzulli}, Gabriele and {Naidu}, Rohan P. and {Ishikawa}, Yuzo and {Brammer}, Gabriel B. and {Chang}, Seok-Jun and {Chisholm}, John and {de Graaff}, Anna and {D'Eugenio}, Francesco and {Di Cesare}, Claudia and {Eilers}, Anna-Christina and {Greene}, Jenny E. and {Gronke}, Max and {Iani}, Edoardo and {Kokorev}, Vasily and {Kotiwale}, Gauri and {Kramarenko}, Ivan and {Ma}, Yilun and {Mascia}, Sara and {Navarrete}, Benjam{\'\i}n and {Nelson}, Erica and {Oesch}, Pascal and {Simcoe}, Robert A. and {Wuyts}, Stijn},
  title = {{The warm outer layer of a little red dot as the source of [Fe II] and collisional Balmer lines with scattering wings}},
  journal = {\aap},
  keywords = {galaxies: active, galaxies: high-redshift, galaxies: nuclei, quasars: supermassive black holes},
  year = {2026},
  month = feb,
  volume = {707},
  eid = {A75},
  pages = {A75},
  doi = {10.1051/0004-6361/202557537},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2026A\&A...707A..75T},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {black hole mass, emission lines, jwst, obscuration, spectroscopy},
  eprint = {2510.00103},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  month_numeric = {2}
}

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