A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z ≲ 2
A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z ≲ 2
Abstract The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies since z ∼ 1 can help to diagnose the origins of locally observed correlations between SMBH mass and stellar mass. We therefore construct three samples of elliptical galaxies, one at z ∼ 0 and two at …