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Far Infrared Emission from an Intergalactic Dust Cloud?

Published online by Cambridge University Press:  08 February 2017

Bogdan Wszolek ,
Konrad Rudnicki ,
Sivia Masi  and
Paolo de Bernardis
Bogdan Wszolek
Affiliation:
Jagellonian University Observatory Cracow, Poland
Konrad Rudnicki
Affiliation:
Jagellonian University Observatory Cracow, Poland
Sivia Masi
Affiliation:
Department of Physics University “La Sapienza” Rome, Italy
Paolo de Bernardis
Affiliation:
Department of Physics University “La Sapienza” Rome, Italy

Extract

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The possible presence of general extragalactic extinction has been studied by many authors. Extragalactic dust can be associated with a pregalactic star population and/or it can be ejected by galaxies during their evolution.

Type
IV. Extragalactic Background Radiation and Cosmology
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 385 - 386
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

de Lapparent, V., Geller, M., and Huchra, J. 1986, Ap. J. (Letters), 302, L1.Google Scholar
Hauser, M. G. et al. 1987, Ap. J. (Letters), 278, L15.Google Scholar
Laurejis, R. J., Mattila, K., and Schnur, G. 1987, Astron. Astrophys., 184, 269.Google Scholar
Murawski, W. 1983, Acta Cosmol., 12, 7.Google Scholar
Okroy, R. 1965, Astron. Cirk., 320, 4.Google Scholar
Rudnicki, K. and Wszolek, B. 1986, in Gamow Cosmology, Proc. of the int. school of physics, E. Fermi Course LXXXVI, eds. Melchiorri, F. and Ruffini, R., North Holland.Google Scholar