Pulsational mass loss from supermassive stars creates the compact shells of Little Red Dots
BibTeX Entry
@article{2026arXiv260419988N,
author = {{Nandal}, Devesh and {Chilingarian}, Igor and {Nagele}, Chris and {Chisholm}, John and {Bauer}, Franz E. and {Loeb}, Abraham},
title = {{Pulsational mass loss from supermassive stars creates the compact shells of Little Red Dots}},
journal = {arXiv e-prints},
keywords = {High Energy Astrophysical Phenomena, Astrophysics of Galaxies, Solar and Stellar Astrophysics},
year = {2026},
month = apr,
eid = {arXiv:2604.19988},
pages = {arXiv:2604.19988},
archiveprefix = {arXiv},
eprint = {2604.19988},
primaryclass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260419988N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {exotic physics, obscuration, simulation, spectroscopy, theory},
month_numeric = {4}
}
Back to bibliography