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Ryo Sawada
Ryo Sawada
Kyoto Sangyo University
Supernova
Physics
late phase
continuous injection
Astrophysics
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A Consistent Modeling of Neutrino-driven Wind with Accretion Flow onto a Protoneutron Star and its Implications for $^{56}$Ni Production.
2020
arXiv: High Energy Astrophysical Phenomena
Ryo Sawada
Yudai Suwa
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