A Fossil Record of Galaxy Encounters
David Elbaz,1*
Catherine J. Cesarsky2
The cosmic infrared background (CIRB) is a record of a large
fraction of the emission of light by stars and galaxies over time. The
bulk of this emission has been resolved by the Infrared Space
Observatory camera. The dominant contributors are bright starburst
galaxies with redshift z ~ 0.8; that is, in the same redshift range as the active galactic nuclei responsible for the bulk
of the x-ray background. At the longest wavelengths, sources of
redshift z
2 tend to dominate the CIRB. It appears
that the majority of present-day stars have been formed in dusty
starbursts triggered by galaxy-galaxy interactions and the buildup of
large-scale structures.
1 Service d'Astrophysique/CEA, CE Saclay,
F-91191 Gif-sur-Yvette, France.
2 European Southern
Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei
München, Germany.
*
To whom correspondence should be addressed. E-mail:
delbaz{at}cea.fr