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Survival of Population III stars
Proceedings of the International Astronomical Union, 2018AbstractIn our earlier studyDutta (2016a), it has been shown that a number of primordial protostars (the ‘first stars’ in the Universe, also known as Population III or Pop III stars) are being ejected from the cluster of their origin with the velocity exceeding their escape velocity.
Jayanta Dutta +3 more
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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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Nucleosynthesis in Aspherical Explosions of Population III Stars
AIP Conference Proceedings, 2008We present the nucleosynthetic yields of Population III core‐collapse supernovae (SNe) focusing on the cases of hyper‐energetic (Hypernovae, HNe) and hyper‐aspherical (jet‐induced) explosions. We show that (1) the explosions with large energy deposition rate, Ėdep, are observed as GRB‐HNe and their yields can explain the abundances of normal extremely ...
Nomoto, K. +4 more
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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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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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Cancer statistics for the US Hispanic/Latino population, 2021
Ca-A Cancer Journal for Clinicians, 2021Kimberly D Miller +2 more
exaly
Population‐based programs for increasing colorectal cancer screening in the United States
Ca-A Cancer Journal for Clinicians, 2015Richard C Wender
exaly
Management of Lung Cancer in Older Adults
Ca-A Cancer Journal for Clinicians, 2003Arti Hurria, Mark Kris
exaly