Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-05-16T04:49:49.452Z Has data issue: false hasContentIssue false
  • English
  • Français

The Infrared Background Due to Galaxies

Published online by Cambridge University Press:  08 February 2017

F.-X. Désert  and
J. -L Puget
F.-X. Désert
Affiliation:
Laboratory Astrophysics Huygens Laboratorium N. Bohrweg 2 Postbus 9504 2300 RA LEIDEN The Netherlands
J. -L Puget
Affiliation:
Groupe de Radioastronomie E. N. S. 24 rue Lhomond 75231 Paris Cedex 5 France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have investigated the galactic infrared background (GIRB) light that comes from the integrated emission of individual galaxies at different redshifts. By using (1) the galaxy M 82 infrared (IR) spectrum as a template spectrum of IR active galaxies and (2) the constraint given by the nucleosynthesis of the heavy elements in galaxies, we have derived the IR spectrum of the diffuse light that comes from the galaxies at different redshifts following the method by Stecker, Puget, and Fazio (1977). The observations by Matsumoto et al. (1988) impose severe constraints on the possible scenarios for the birth and evolution of the galaxies. Observations by the COBE satellite are expected to settle some important issues of this problem.

Type
IV. Extragalactic Background Radiation and Cosmology
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 381 - 382
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Boulanger, F. and Pérault, F. 1988, Ap. J., 330, 848.CrossRefGoogle Scholar
Fabbri, R. et al. 1986, in Proceed, of Marcel Grossman Meeting, Rome, June 1985.Google Scholar
Giard, M. et al., 1989, in Proc. IAU 139, ed. Bowyer, S., Leinert, Ch. (Dordrecht, Kluwer).Google Scholar
Gillett, et al. 1975, Ap. J. (Letters), 198, L75.CrossRefGoogle Scholar
Guiderdoni, B. and Rocca-Volmerange, B. 1989, in Proc. IAU 139, ed. Bowyer, S., Leinert, Ch. (Dordrecth, Kluwer).Google Scholar
Hauser, M. G. et al. 1984, Ap. J. (Letters), 278, L15.CrossRefGoogle Scholar
Jaffe, et al. 1984, Ap. J. (Letters), 285, L31.CrossRefGoogle Scholar
Lange, et al. 1989, in IAU Symp. 135 on Interstellar Dust, ed. Allamandola, L., in press.Google Scholar
Matsumoto, et al. 1988, Ap. J., 329, 567.CrossRefGoogle Scholar
Pajot, F. et al. 1986, Astron. Astrophys., 154, 55.Google Scholar
Puget, J.-L. 1976, COBE report.Google Scholar
Sellgren, K. et al. 1985, Ap. J., 299, 416.CrossRefGoogle Scholar
Soifer, B. T. et al. 1986, Ap. J. (Letters), 303, 141.CrossRefGoogle Scholar
Stecker, F. W., Puget, J.-L., and Fazio, G. 1977, Ap. J. (Letters), 244, L51.CrossRefGoogle Scholar
Telesco, and Harper, 1980, Ap. J., 235, 392.CrossRefGoogle Scholar
Yang, J. et al. 1984, Ap. J., 281, 493.CrossRefGoogle Scholar