Skip to main content

The Cosmic Infrared Background (CIRB) and the Role of the “Local Environment of Galaxies” in the Origin of Present-Day Stars

  • Conference paper
  • First Online:
Multiwavelength Mapping of Galaxy Formation and Evolution

Abstract

A combination of evidence is presented suggesting that the majority of the stars in today’s galaxies were born during a luminous infrared phase (LIRP) triggered by the local environment of galaxies. The CIRB is a fossil record of these LIRPs and therefore reflects the influence of triggered star formation through galaxy-galaxy interactions, including non merging tidal encounters. This scenario, in which galaxies experienced several LIRPs in their history, is consistent with the measured redshift evolution of the cosmic density of star formation rates and of stellar masses of galaxies.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Author information

Authors and Affiliations

Authors

Editor information

Alvio Renzini Ralf Bender

Rights and permissions

Reprints and permissions

About this paper

Cite this paper

Elbaz, D., Marcillac, D., Moy, E. The Cosmic Infrared Background (CIRB) and the Role of the “Local Environment of Galaxies” in the Origin of Present-Day Stars. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_2

Download citation

Publish with us

Policies and ethics