A quasi-star is born: formation and evolution of accreting quasi-stars as a metallicity-independent pathway to Little Red Dots
BibTeX Entry
@article{2026arXiv260321714R,
author = {{Roman-Garza}, J. and {Schaerer}, D. and {Charbonnel}, C. and {Fragos}, T. and {Cenci}, E. and {Marques-Chaves}, R. and {Oesch}, P. and {Xiao}, M.},
title = {{A quasi-star is born: formation and evolution of accreting quasi-stars as a metallicity-independent pathway to Little Red Dots}},
journal = {arXiv e-prints},
keywords = {Solar and Stellar Astrophysics, Astrophysics of Galaxies, High Energy Astrophysical Phenomena},
year = {2026},
month = mar,
eid = {arXiv:2603.21714},
pages = {arXiv:2603.21714},
archiveprefix = {arXiv},
eprint = {2603.21714},
primaryclass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260321714R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, exotic physics, simulation, super-eddington, theory},
month_numeric = {3}
}
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