2003/03/20 by P. T. de Zeeuw, Tim de Zeeuw, de Zeeuw, Tim
Physics and Astronomy · #Astrophysics (astro-ph) #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #Relativity and Gravitational Theory #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0303469
12 pages, LaTeX, no figures. To appear in: Carnegie Observatories Astrophysics Series, Vol. 1: Coevolution of Black Holes and Galaxies, ed. L. C. Ho (Cambridge: Cambridge Univ. Press)
openalex publication_date 2003/03/20 · arxiv created 2003/05/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
In the past decade, much effort was devoted to measure the masses of supermassive black holes in galactic nuclei, to establish the relation between black hole mass and the global/nuclear properties of the host galaxy, and to understand the role of these objects in the formation and subsequent dynamical evolution of galaxies. This whole area of research is an appropriate and timely topic for the first in this series of symposia. Nearly half the contributions were devoted to the various methods that are being used to estimate masses of central black holes, from nearby globular clusters all the way to quasars at redshifts z>6. This work forms the foundation of our understanding of black hole demography, and provides constraints on scenarios for black hole formation and growth, and on their connection to the formation and properties of the host galaxy. I will address these topics in this same order.