# The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences

@article{Dullo2020TheH,
title={The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences},
author={B. T. Dullo and A. Bouquin and A. Paz and J. Knapen and J. Gorgas},
journal={arXiv: Astrophysics of Galaxies},
year={2020}
}
[Abridged] Tight correlations between supermassive black hole (SMBH) mass ($M_{\rm BH}$) and the properties of the host galaxy have useful implications for our understanding of the growth of SMBHs and evolution of galaxies. Here, we present newly observed correlations between $M_{\rm BH}$ and the host galaxy total UV$-$ [3.6] color ($\mathcal{C_{\rm UV,tot}}$, Pearson's r = $0.6-0.7$) for a sample of 67 galaxies (20 early-type galaxies and 47 late-type galaxies) with directly measured \$M_{\rm… Expand
2 Citations