A Physical Model for the joint evolution of high-z QSOs and Spheroids

Simple item page
dc.creatorGranato, Gian Luigi
dc.creatorSilva, Laura
dc.creatorDanese, Luigi
dc.creatorDe Zotti, Gianfranco
dc.creatorBressan, Alessandro
dc.date2005-04-21
dc.date.accessioned2026-07-07T02:17:30Z
dc.date.available2026-07-07T02:17:30Z
dc.descriptionWe summarize our physical model for the early co-evolution of spheroidal galaxies and of active nuclei at their centers. Our predictions are in excellent agreement with a number of observables which proved to be extremely challenging for all the current semi-analytic models, including the sub-mm counts and the corresponding redshift distributions, and the epoch-dependent K-band luminosity function of spheroidal galaxies. Also, the black hole mass function and the relationship between the black hole mass and the velocity dispersion in the galaxy are nicely reproduced. The mild AGN activity revealed by X-ray observations of SCUBA sources is in keeping with our scenario, and testify the build up of SMBH triggered by intense star formation.
dc.description6 Pages, 5 figures, Invited talk at "Multiwavelength AGN surveys", Cozumel, Mexico, December 2003, eds. R. Mujica & R. Maiolino, Singapore: World Scientific, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0504473
dc.identifierhttp://arxiv.org/abs/astro-ph/0504473
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9195
dc.subjectAstrophysics
dc.titleA Physical Model for the joint evolution of high-z QSOs and Spheroids
dc.typetext

Files

Collections

arXiv