Constraints on massive black holes as dark matter candidates using Galactic globular clusters

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 3, 1996, Pages 735-748

  Klessen, Ralf ^a,b   Burkert, Andreas ^a,b  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Black hole physics; Dark matter; Galaxy: halo; Globular clusters: general

Indexed keywords

BLACK HOLES; GRAVITATION; INTELLIGENT SYSTEMS; MONTE CARLO METHODS; POPULATION STATISTICS; STARS;

BLACK HOLE MASS; BLACK HOLE PHYSICS; DARK MATTER; DARK MATTER HALOS; EXPOSED TO; GALAXY:HALO; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; MASSIVE BLACK HOLES; TIME-SCALES;

GALAXIES;

EID: 0040632674     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.3.735     Document Type: Article

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