= Luis C. Ho
{c}
<Luis C. Ho> investigates <supermassive black holes> and their connections to host <galaxies>. His review with <John Kormendy> organized dynamically measured <black hole> <mass>[masses] by host structure, including classical bulges, <galactic disks> and <pseudobulges>.
The distinction changes the physical interpretation of a scaling relation. Strong correlations with some bulge properties do not establish equally close coupling to every component of a <galaxy>. The review argued that weak relations for <galactic disks> and <pseudobulges> require a richer account of <black hole> growth than a single universal coevolution rule.<Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies by John Kormendy and Luis C. Ho>[Abstract: dynamically measured demographics, component-dependent correlations and proposed growth regimes]{ref}
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{title=Portrait of <Luis C. Ho>}
{description=External portrait hosted by Kavli Institute for Astronomy and Astrophysics, Peking University.}
{source=https://kiaa.pku.edu.cn/info/1031/8910.htm}
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