Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24..579s&link_type=abstract
(Astrofizika, vol. 24, May-June 1986, p. 579-590) Astrophysics (ISSN 0571-7132), vol. 24, no. 3, Nov. 1986, p. 331-338. Translat
Astronomy and Astrophysics
Astrophysics
1
Background Radiation, Infrared Radiation, Protostars, Radiant Flux Density, Stellar Radiation, Interstellar Matter, Near Infrared Radiation, Red Giant Stars, Stellar Evolution, Stellar Mass, Supernovae
Scientific paper
The spectrum of infrared background radiation produced by primordial stars is calculated. On the assumption that these stars enrich matter by heavy elements in quantities typical for population II stars, it is shown that the infrared radiation flux will be about 50 Jy/sr in the wavelength interval 15-30 microns and about 200 Jy/sr in the interval 150-300 microns. The background radiation flux in the near-infrared range from low-mass population II stars and massive population III stars is estimated. It is shown that it is too small in comparison with the observable fluxes.
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