Cosmic Outliers: Low-spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
BibTeX Entry
@article{2025ApJ...989L..19P,
author = {{Pacucci}, Fabio and {Loeb}, Abraham},
title = {{Cosmic Outliers: Low-spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots}},
journal = {\apjl},
keywords = {Early universe, Galaxies, Cosmology, Galaxy evolution, Active galaxies, 435, 573, 343, 594, 17, Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2025},
month = aug,
volume = {989},
number = {2},
eid = {L19},
pages = {L19},
doi = {10.3847/2041-8213/ade871},
archiveprefix = {arXiv},
eprint = {2506.03244},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025ApJ...989L..19P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
altmetric = {180223611},
lrdkeys = {clustering, early universe, jwst, morphology, theory},
month_numeric = {8}
}
Back to bibliography