SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 330, L37-L40 (1998)


Table of Contents
Available formats: HTML | PDF | (gzipped) PostScript

Letter to the Editor

Are ultra-luminous infrared galaxies
the dominant extragalactic population at high luminosities?

Gopal Krishna 1 and Peter L. Biermann 2

1 National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune University Campus, Pune 411007, India
2 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany (e-mail: plbiermann@mpifr-bonn.mpg.de)

Received 29 August 1997 / Accepted 20 November 1997

Abstract

Based on the recent QSO surveys it is shown that, contrary to the widespread notion, high-luminousity QSOs are at least as numerous in the nearby universe as the ultraluminous far-infrared galaxies (ULIGs). Therefore, the fraction of ULIGs that have got a hidden quasar at the nucleus, for example in the dust shrouded phase, cannot be overwhelmingly large.

Key words: galaxies: interactions – galaxies: luminosity function – galaxies: starburst – galaxies: active – quasars: general – infrared: galaxies

Send offprint requests to: Gopal Krishna
(e-mail: krishna@ncra.tifr.res.in)

© European Southern Observatory (ESO) 1998

Online publication: January 16, 1998
helpdesk.link@springer.de