Obscured active galactic nuclei in luminous infrared galaxies

L. M. Shier, M. J. Rieke, G. H. Rieke

Research output: Contribution to journalArticlepeer-review

46 Scopus citations

Abstract

We examine the nature of the central power source in very luminous infrared galaxies. The infrared properties of the galaxies, including their far-infrared and 2.2 μm fluxes, CO indices, and Brackett line fluxes are compared to models of starburst stellar populations. Among seven galaxies we found two dominated by emission from young stars, two dominated by emission from an AGN, and three transition cases. Our results are consistent with evidence for active nuclei in the same galaxies at other wave-lengths. Nuclear mass measurements obtained for the galaxies indicate an initial mass function biased toward high-mass stars in two galaxies. After demonstrating our methods in well-studied galaxies, we define complete samples of high luminosity and ultraluminous galaxies. We find that the space density of embedded and unembedded quasars in the local universe is similar for objects of similar luminosity. If quasars evolve from embedded sources to optically prominent objects, it appears that the lifetime of a quasar is no more than about 108 yr.

Original languageEnglish (US)
Pages (from-to)222-236
Number of pages15
JournalAstrophysical Journal
Volume470
Issue number1 PART I
DOIs
StatePublished - Jan 1 1996

Keywords

  • Galaxies: Active
  • Galaxies: Evolution
  • Galaxies: Starburst
  • Galaxies: Stellar content
  • Infrared: Galaxies
  • Quasars: General

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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