Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots
BibTeX Entry
@article{2025arXiv251217997C,
author = {{Cantiello}, Matteo and {Hassan}, Jake B. and {Perna}, Rosalba and {Armitage}, Philip J. and {Begelman}, Mitchell C. and {Jiang}, Yan-Fei and {Ryu}, Taeho and {Townsend}, Richard H. D.},
title = {{Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots}},
journal = {arXiv e-prints},
keywords = {High Energy Astrophysical Phenomena, Astrophysics of Galaxies, Solar and Stellar Astrophysics},
year = {2025},
month = dec,
eid = {arXiv:2512.17997},
pages = {arXiv:2512.17997},
archiveprefix = {arXiv},
eprint = {2512.17997},
primaryclass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv251217997C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, early universe, jwst, theory, variability},
month_numeric = {12}
}
Back to bibliography