Supernovae in massive binaries and compact object mergers near supermassive black holes

Nuclear star clusters that surround supermassive black holes (SMBHs) in galactic nuclei are among the densest systems in the Universe, harbouring millions of stars and compact objects (COs). Within a few parsecs from the SMBH, stars can form binaries. In this paper, we model the supernova (SN) proce...

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Veröffentlicht in:	Journal of cosmology and astroparticle physics 2019-10, Vol.2019 (10), p.45-45
Hauptverfasser:	Fragione, Giacomo, Ginsburg, Idan, Loeb, Abraham
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Computer simulation Galactic nuclei Gravitational waves Gravity waves Star clusters Supermassive black holes Supernovae
Online-Zugang:	Volltext
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