Non-LTE radiative transfer models of very luminous sources and their applicability to little red dots, quasi-stars, and similar objects
BibTeX Entry
@article{2026A&A...713A.285M,
author = {{Martins}, Fabrice and {Schaerer}, Daniel and {Marques-Chaves}, Rui},
title = {{Non-LTE radiative transfer models of very luminous sources and their applicability to little red dots, quasi-stars, and similar objects}},
journal = {\aap},
keywords = {stars: atmospheres, quasars: supermassive black holes},
year = {2026},
month = sep,
volume = {713},
eid = {A285},
pages = {A285},
doi = {10.1051/0004-6361/202660767},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026A\&A...713A.285M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
month_numeric = {9}
}
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