Observational manifestations of population III stars

Details Observational manifestations of population III stars Observational manifestations of population III stars

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25..559v&link_type=abstract

(Astrofizika, vol. 25, Nov.-Dec. 1986, p. 559-572) Astrophysics (ISSN 0571-7132), vol. 25, no. 3, May 1987, p. 680-688. Translat

Astronomy and Astrophysics

Astrophysics

Gas Heating, High Temperature Gases, Microwave Spectra, Nuclear Fusion, Stellar Activity, X Ray Spectra, Background Radiation, Deuterium, Gas Cooling, Light Elements, Lithium

Scientific paper

The thermal history of gas heated by explosions of population III stars at redshifts z of about 100 is calculated. The distortions in the spectrum of the microwave radiation and the intensity of the resulting X-rays are determined. Bounds on the energy release produced by the explosions of such stars are compared with available observations. The possibility of synthesis of light elements in very massive primordial stars is discussed.

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