Simulation of a population of isolated neutron stars evolving through the emission of gravitational waves

Monthly Notices of the Royal Astronomical Society

Volumn 359, Issue 3, 2005, Pages 1150-1164

  Palomba, C ^a  

^a INFN SEZIONE DI ROMA   (Italy)

Author keywords

Gravitational waves; Stars: neutron; Stars: statistics

Indexed keywords

GRAVITATIONAL EFFECTS; INTELLIGENT SYSTEMS; MONTE CARLO METHODS; NEUTRONS; POPULATION STATISTICS; STARS;

DYNAMICAL EVOLUTION; GOULD BELT; GRAVITATIONAL POTENTIAL; ISOLATED NEUTRON STARS; MAGNETIC-FIELD; MONTE CARLO'S SIMULATION; NEUTRON STARS; STAR FORMATION RATES; STARS: NEUTRONS; STARS: STATISTICS;

GRAVITY WAVES;

EID: 19844373156     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08975.x     Document Type: Article

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