The Black Hole Mass-Color Relations for Early- and Late-type Galaxies: Red and Blue Sequences
The tight correlations between supermassive black hole (SMBH) mass (M BH) and the properties of the host galaxy have useful implications for our understanding of the growth of SMBHs and of the evolution of galaxies. Here, we present newly observed correlations between M BH and the host galaxy total UV-[3.6] color ( ${{ \mathcal C }}_{\mathrm{UV}
Dullo, Bililign T. et al.
Fecha de publicación:
7
2020