Little Red Dots as self-gravitating discs accreting on supermassive stars: Spectral appearance and formation pathway of the progenitors to direct collapse black holes
BibTeX Entry
@article{2025arXiv250722014Z,
author = {{Zwick}, Lorenz and {Tiede}, Christopher and {Mayer}, Lucio},
title = {{Little Red Dots as self-gravitating discs accreting on supermassive stars: Spectral appearance and formation pathway of the progenitors to direct collapse black holes}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2025},
month = jul,
eid = {arXiv:2507.22014},
pages = {arXiv:2507.22014},
archiveprefix = {arXiv},
eprint = {2507.22014},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250722014Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, non-agn, sed, spectroscopy, theory},
month_numeric = {7}
}
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