Gas accretion versus black-hole-merger-driven growth modes of supermassive black holes and implications for the little red dots
BibTeX Entry
@article{2026A&A...709A...9B,
author = {{Barai}, Paramita},
title = {{Gas accretion versus black-hole-merger-driven growth modes of supermassive black holes and implications for the little red dots}},
journal = {\aap},
keywords = {black hole physics, hydrodynamics, methods: numerical, galaxies: formation, quasars: supermassive black holes, Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2026},
month = apr,
volume = {709},
eid = {A9},
pages = {A9},
doi = {10.1051/0004-6361/202558028},
archiveprefix = {arXiv},
eprint = {2602.15952},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026A\&A...709A...9B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
month_numeric = {4}
}
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