Dot to dot: high-z little red dots in M_\rm bh-M_\rm ⋆ diagrams with galaxy-morphology-specific scaling relations and nuclear star clusters
BibTeX Entry
@article{2025arXiv250310958G,
author = {{Graham}, Alister W. and {Chilingarian}, Igor V. and {Nguyen}, Dieu D. and {Soria}, Roberto and {Durre}, Mark and {Forbes}, Duncan A.},
title = {{Dot to dot: high-$z$ little red dots in $M\_{\rm bh}$-$M\_{\rm \star}$ diagrams with galaxy-morphology-specific scaling relations and nuclear star clusters}},
journal = {arXiv e-prints},
keywords = {Astrophysics - Astrophysics of Galaxies},
year = {2025},
month = mar,
eid = {arXiv:2503.10958},
pages = {arXiv:2503.10958},
doi = {10.48550/arXiv.2503.10958},
archiveprefix = {arXiv},
eprint = {2503.10958},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250310958G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, early universe, host galaxy, jwst, morphology},
month_numeric = {3}
}
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