A new formation channel for double neutron stars without recycling: Implications for gravitational wave detection

Astrophysical Journal

Volumn 550, Issue 2 PART 2, 2001, Pages

  Belczyński, Krzysztof ^a,b   Kalogera, Vassiliki ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

Author keywords

Binaries: close; Gravitational waves; Stars: evolution; Stars: formation; Stars: neutron

Indexed keywords

EID: 0035314969     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/319641     Document Type: Article

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