Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN
BibTeX Entry
@article{2026arXiv260110573A,
author = {{Asada}, Yoshihisa and {Inayoshi}, Kohei and {Fei}, Qinyue and {Fujimoto}, Seiji and {Willott}, Chris},
title = {{Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies},
year = {2026},
month = jan,
eid = {arXiv:2601.10573},
pages = {arXiv:2601.10573},
archiveprefix = {arXiv},
eprint = {2601.10573},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260110573A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {early universe, emission lines, jwst, sed, starburst},
month_numeric = {1}
}
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