A comprehensive study of binary compact objects as gravitational wave sources: Evolutionary channels, rates, and physical properties

Astrophysical Journal

Volumn 572, Issue 1 I, 2002, Pages 407-431

  Belczynski, Krzysztof ^a,b,c   Kalogera, Vassiliki ^a,b   Bulik, Tomasz ^c  

^a NORTHWESTERN UNIVERSITY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

Author keywords

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

Indexed keywords

EID: 0000323345     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/340304     Document Type: Review

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