Predictions for triple stars with and without a pulsar in star clusters

Monthly Notices of the Royal Astronomical Society

Volumn 387, Issue 2, 2008, Pages 815-824

  Trenti, Michele ^a   Ransom, Scott ^b   Hut, Piet ^c   Heggie, Douglas C ^d  

^a AURA for the European Space Agency   (United States)

^b NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^c INSTITUTE FOR ADVANCED STUDY   (United States)

^d UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

Globular clusters: general; Methods: N body simulations; Pulsars: general; Stellar dynamics

Indexed keywords

MASS SPECTROMETRY; PULSARS;

DIRECT SIMULATION; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; MASS STARS; METHODS:N-BODY SIMULATIONS; MOST LIKELY; PULSARS: GENERAL; STAR CLUSTERS; STELLAR DYNAMICS; TRIPLE SYSTEM;

FORECASTING;

EID: 45149133457     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13285.x     Document Type: Article

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