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Chiaki, G.
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Chiaki, G.
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Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
by
Chiaki
,
G
.
,
Kinugawa, T.
,
Suwa, Y.
,
Tanikawa, A.
,
Tominaga, N.
Published 2022
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Related Subjects
Black holes
Cosmology
Efficiency
Gravitation
Gravitational-waves
Merging
Metal free
Metal-poor star
Minimum mass
Stars formation
Stars: Be
Stars: Population II
Stars: Population III
Stars: black holes
Supernovae
gravitational waves
stars: Population II
stars: Population III
stars: black holes
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