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Quasars, Starbursts, and the Cosmic Energy Budget
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1
QUASARS, STARBURSTS, AND THE COSMIC ENERGY BUDGET
A. Lawrence
Institute for Astronomy, University of Edinburgh,
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ,
Scotland, UK
Abstract
Observations in the far infrared are the best way to
make an unbiased survey of active galaxies in the loosest
sense - but separating the the true quasars from the sur-
rounding starburst may be difficult. There is in fact much
evidence to suggest that starburst and AGN activity are
intimately connected, and FIRST will help us to explore
this link. Since the last major FIRST conference in Greno-
ble, this issue has become even more central to modern
astrophysics, with the realisation of the dominance of the
FIR background, the discovery of high redshift SCUBA
sources, and the emergence of the black hole mass deficit
problem. What dominates the cosmic energy budget - nu-
clear fusion or accretion ?
Key words: Cosmology:observations - Quasars:X-rays - Galax-
ies:starburst - Galaxies:formation
1. Introduction
The FIRST mission will make important contributions to
AGN studies in several ways. Broad-band colours could be
measured for hundreds of selected AGN of various types,
including AGN at much higher redshift than previously
possible. Spectral energy distributions could be measured
for dozens of objects. Blazar monitoring could be per-
formed at sub-mm wavelengths, measuring changes in the
real core, rather than pc-scale jets. Very large numbers
of submm selected AGN will come from the anticipated
survey programmes. The issues addressed by such studies
include AGN dust models, the starburst/AGN ratio, and
its variation with luminosity, redshift, radio power etc, and
the question of when dust first formed.
The prospect for most of the above issues has not
changed much since the last conference looking forward to
FIRST, in Grenoble 1997. (Lawrence 1997). However the
FIR emission from AGN has taken on a new cosmol
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