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Gravitational wave sources from Pop III stars are preferentially located within the cores of their host Galaxies

Gravitational wave sources from Pop III stars are preferentially located within the cores of their host Galaxies

Pacucci, Fabio; Loeb, Abraham; Salvadori, Stefania
  • 期刊名称Monthly Notices of the Royal Astronomical Society: Letters
  • 作者Pacucci, Fabio; Loeb, Abraham; Salvadori, Stefania
  • 卷第471卷
  • 期第1期
  • 印刷ISSN1745-3925
  • 电子ISSN1745-3933
  • 文件大小432.52KB
  • 发表时间2017-10-11
  • DOI10.1093/mnrasl/slx111
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