Constraining population synthesis models via empirical binary compact object merger and supernova rates

Astrophysical Journal

Volumn 672, Issue 1, 2008, Pages 479-488

  O'Shaughnessy, R ^a   Kim, C ^b   Kalogera, V ^a   Belczynski, K ^c  

^a NORTHWESTERN UNIVERSITY   (United States)

^b Department of Obstetrics Gynecology   (United States)

^c NEW MEXICO STATE UNIVERSITY   (United States)

Author keywords

Binaries: close; Black hole physics; Stars: evolution; Stars: neutron

Indexed keywords

EID: 40249111531     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/523620     Document Type: Article

References (66)