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Observational manifestations of population III stars
Astrophysics, 1987The thermal history of gas heated by explosions of population III stars at red shifts z approx. 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.
B. V. Vainer +2 more
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GRAVITATIONAL COLLAPSE OF POPULATION III STARS
The Eleventh Marcel Grossmann Meeting, 2008▌ The expected diffuse cosmic neutrino flux produced by Pop III stars during their nuclear burning and their core-collapse phases▌ Estimated flux is comparable to the diffuse neutrino fluxes produced by ordinary SNe. However, due to the large cosmological redshift, the typical energies are MeV and sub-MeV, where the other components dominate.
YUDAI SUWA +3 more
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Evolution and Nucleosynthesis in Population III Stars
1982In recent years many arguments have been gathered in favour of the existence of a pregalactic generation of very massive objects (VMOs). An early generation of massive stars, which become pair unstable at the end of their evolution (M > 80 Mo) may manifest itself by its influence on the galactic chemical abundances and on the intensity and spectral ...
W. W. Ober, M. F. Eid, K. J. Fricke
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Nucleosynthetic Consequences of Population III Stars
1986It is argued that the Population III stars with the most explanatory power are Very Massive Objects (VMOs) in the mass range ...
B. J. Carr, W. Glatzel
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On the Properties of Population III Stars and “Galaxies”
2002We present new model calculations for massive Population III stars and metal-free stellar populations. The properties of individual stars and integrated populations, including their ionizing fluxes, SEDs, and baryon production are discussed. We also study their dependence on the poorly known IMF and the star formation history.
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Diversity of Population III Star Formation
2019The aim of this thesis is to improve our understanding of the fragmentation behavior of Population III protostellar disks under the influence of rotation, turbulence, and magnetic fields. We further evaluate consequences that may be inferred for the later evolution of the star-forming halo and its surroundings with respect to protostellar ejections and
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Gravitational wave of intermediate-mass black holes in Population III star clusters
Monthly Notices of the Royal Astronomical Society, 2022Michiko S Fujii, Ataru Tanikawa
exaly
Trapping of H ii regions in Population III star formation
Monthly Notices of the Royal Astronomical Society, 2022Lionel Haemmerlé +2 more
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Massive binary black holes from Population II and III stars
Monthly Notices of the Royal Astronomical Society, 2023Michela Mapelli +2 more
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Primordial magnetic fields in Population III star formation: a magnetized resolution study
Monthly Notices of the Royal Astronomical Society, 2022Simon Glover, Ralf Klessen, Paul C Clark
exaly