Results 101 to 110 of about 3,128 (211)
Metal-enriched Pair-instability Supernovae: Effects of Rotation
The Astrophysical JournalIn this paper, we revisit metal-enriched rotating pair-instability supernovae (PISNe) models for metallicities consistent with the Small Magellanic Cloud, the Large Magellanic Cloud (LMC), and 0.1 Z _⊙ .
Hideyuki Umeda, Chris Nagele
doaj +1 more source
EPJ Web of Conferences, 2016 The experimental B(GT) strengths of the 59Fe excited states were employed to determine the transition strengths which greatly contribute 59Fe stellar β–decay at typical carbon shell burning temperature.
Li K. +4 more
doaj +1 more source
Topics in Core-Collapse Supernova Theory: The Formation of Black Holes and the Transport of Neutrinos [PDF]
, 2012 Core-Collapse Supernovae are one of the most complex astrophysical systems in the universe. They deeply entwine aspects of physics and astrophysics that are rarely side by side in nature.
O'Connor, Evan Patrick
core +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page i-xlii, August 2024.
wiley +2 more sources
Role of clusters in nuclear astrophysics with Cluster Nucleosynthesis Diagram (CND)
, 2020 The role of nuclear clustering in stellar reactions is discussed, with Cluster Nucleosynthesis Diagram (CND) proposed before, for nucleosynthesis in stellar evolution and explosive stellar phenomena.
한인식
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STUDY OF ASTROPHYSICAL NUCLEAR REACTIONS AND THEIR ROLE IN STELLAR EVOLUTION
Worldwide Journal of PhysicsAstrophysical nuclear reactions are fundamental to the life cycle of stars and the chemical evolution of the universe. This study investigates the critical nuclear processes occurring within stellar environments, including the proton-proton chain, the ...
Syed Rizwan Hussain +1 more
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Nucleosynthesis by N-14 depletion during shell He burning in massive stars
, 1987 New computations of He shell nucleosynthesis occurring during both radiative and convective phases are presented for stars in the range 8 - 25 M_sun;, taking in account the recent changes proposed for many cross sections.
R. Gallino +3 more
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Simulating molecular cloud regulated star formation in Galaxies [PDF]
, 2007 This thesis is primarily concerned with understanding the process of galaxy formation via the simulation of the interstellar medium, star formation and supernova feedback.
Booth, Craig Martin
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Nucleosynthesis and Nucleo-Cosmochronology
, 2004 I discuss a few selected topics on nucleosynthesis and nucleo-cosmochronology in faint, if not totally illusory, hopes of helping to gain a clear perspective of the future astronuclear physics.
K. Takahashi
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Molecular hydrogen in galaxies [PDF]
, 1987 This study aims to understand the key role played by molecular hydrogen in the evolution of galaxies, with a view to constraining its radial distribution in the Galaxy and the CO→H(_2) conversion factor α(_20).The star formation rate is shown to be ...
Wilkinson, David Adam, Wilkinson, D.A
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