Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'501'711
Articles rated: 2609

19 April 2024
 
  » arxiv » astro-ph/0603819

 Article overview


Quasar Luminosity Functions from Joint Evolution of Black Holes and Host Galaxies
A. Lapi ; F. Shankar ; J. Mao ; G.L. Granato ; L. Silva ; G. De Zotti ; L. Danese ;
Date 30 Mar 2006
AbstractWe show that our anti-hierarchical baryon collapse scenario (Granato et al. 2004) for the joint evolution of black holes and host galaxies predicts quasar luminosity functions at redshifts 1.5 < z < 6 and local demographic properties in nice agreement with observations. In our model the quasar activity marks and originates the transition between an earlier phase of violent and heavily dust-enshrouded starburst activity promoting rapid black hole growth, and a later phase of almost passive evolution; the former is traced by the submillimeter-selected sources, while the latter accounts for the high number density of massive galaxies at substantial redshifts z > 1.5, the population of Extremely Red Objects, and the properties of local ellipticals.
Source arXiv, astro-ph/0603819
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica