The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings

@misc{torralbaFri Oct 03 2025 07:50:53 GMT+0000 (Coordinated Universal Time)warmouterlayer,
      title={The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings},
      author={Alberto Torralba and Jorryt Matthee and Gabriele Pezzulli and Rohan P. Naidu and Yuzo Ishikawa and Gabriel B. Brammer and Seok-Jun Chang and John Chisholm and Anna de Graaff and Francesco D'Eugenio and Claudia Di Cesare and Anna-Christina Eilers and Jenny E. Greene and Max Gronke and Edoardo Iani and Vasily Kokorev and Gauri Kotiwale and Ivan Kramarenko and Yilun Ma and Sara Mascia and Benjamín Navarrete and Erica Nelson and Pascal Oesch and Robert A. Simcoe and Stijn Wuyts},
      year={Fri Oct 03 2025 07:50:53 GMT+0000 (Coordinated Universal Time)},
      eprint={2510.00103},
      archivePrefix={arXiv},
      primaryClass={astro-ph.GA},
      url={https://arxiv.org/abs/2510.00103},
}