Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects
BibTeX Entry
@article{2026arXiv260512141M,
author = {{Martins}, Fabrice and {Schaerer}, Daniel and {Marques-Chaves}, Rui},
title = {{Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies},
year = {2026},
month = may,
eid = {arXiv:2605.12141},
pages = {arXiv:2605.12141},
archiveprefix = {arXiv},
eprint = {2605.12141},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260512141M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
month_numeric = {5}
}
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