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Formation of SMBH seeds in Population III star clusters through collisions: the importance of mass loss
Formation of SMBH seeds in Population III star clusters through collisions: the importance of mass loss
2020
P. J. Alister Seguel
Dominik R. G. Schleicher
T C N Boekholt
Michael Fellhauer
Ralf S. Klessen
Keywords:
Star cluster
Astronomy
Astrophysics
Population
Physics
Correction
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