The Black Hole Mass–Color Relations for Early- and Late-type Galaxies: Red and Blue Sequences

@article{Dullo2020TheBH,
  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. G. de 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
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