Comparative Analysis of Safety and Efficacy: Conventional Mediolateral Pinning vs. Dorgan's Lateral Cross-Pinning in Pediatric Supracondylar Fractures. [PDF]
Khan MW +9 more
europepmc +1 more source
Repeated Extraneous Introductions of Cholera, Thailand, 2007-2025. [PDF]
Okada K +9 more
europepmc +1 more source
Diet Reconstruction Under Limited Prior Information: Dietary Contributions and Isotopic Niche of <i>Metridium senile</i> in the North Yellow Sea. [PDF]
Zhao Y +5 more
europepmc +1 more source
Dairy product consumption and thyroid cancer risk: a systematic review and meta-analysis of observational studies. [PDF]
Song X +6 more
europepmc +1 more source
Subcuticular symbionts of intertidal brittle stars: diversity, host specificity, and functional potential. [PDF]
Kawano K +5 more
europepmc +1 more source
A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
europepmc +1 more source
Related searches:
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
openaire +1 more source
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
openaire +2 more sources
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
openaire +1 more source

