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Gravitational wave sources from Pop III stars are preferent..:
Pacucci, Fabio
;
Loeb, Abraham
;
Salvadori, Stefania
Monthly Notices of the Royal Astronomical Society: Letters. 471 (2017) 1 - p. L72-L76 , 2017
Link:
https://doi.org/10.1093/mnrasl/slx111
RT Journal T1 <Title>Gravitational wave sources from Pop III stars are preferentially located within the cores of their host Galaxies</Title> UL https://suche.suub.uni-bremen.de/peid=cr-10.1093_mnrasl_slx111&Exemplar=1&LAN=DE A1 Pacucci, Fabio A1 Loeb, Abraham A1 Salvadori, Stefania PB Oxford University Press (OUP) YR 2017 SN 1745-3925 SN 1745-3933 JF Monthly Notices of the Royal Astronomical Society: Letters VO 471 IS 1 SP L72 OP L76 LK http://dx.doi.org/https://doi.org/10.1093/mnrasl/slx111 DO https://doi.org/10.1093/mnrasl/slx111 SF ELIB - SuUB Bremen
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