Compact Massive Object in Galaxies
I. Tosta e Melo, R. Capuzzo-Dolcetta

TL;DR
This paper analyzes a large dataset of Compact Massive Objects in galaxies, exploring their properties and correlations with host galaxy characteristics to understand their nature and relationships.
Contribution
It provides a comprehensive analysis of Compact Massive Objects, highlighting their similarities and correlations with host galaxy properties, suggesting a unified understanding.
Findings
Compact Massive Objects correlate with galaxy magnitude and velocity dispersion.
Supermassive black holes and dense stellar clusters may form a continuum.
The study supports the idea of a common family of Compact Massive Objects.
Abstract
The central regions of galaxies show the presence of super massive black holes and/or very dense stellar clusters. Both objects seem to follow similar host-galaxy correlations, suggesting that they are members of the same family of Compact Massive Objects. We investigate here a huge data collection of Compact Massive Objects properties to correlate them with absolute magnitude, velocity dispersion and mass of their host galaxies.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
