Constraints on the mass and abundance of black holes in the Galactic halo: The high-mass limit

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 1, 2000, Pages 87-98

  Murali, Chigurupati ^a,c   Arras, Phil ^b   Wasserman, Ira ^b  

^a UNIVERSITY OF TORONTO   (Canada)

^b Cornell University ^*  (United States)

^c UNIVERSITY OF MASSACHUSETTS   (United States)

Author keywords

Dark matter; Galaxy: halo; Galaxy: structure; Globular clusters: general

Indexed keywords

BLACK HOLES; GALAXIES; GRAVITATION; INTELLIGENT SYSTEMS; MONTE CARLO METHODS;

DARK MATTER; EVOLUTIONARY MODELS; GALACTIC HALO; GALACTOCENTRIC RADIUS; GALAXIES:STRUCTURE; GALAXY:HALO; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; MONTE CARLO'S SIMULATION; SIMPLE++;

STARS;

EID: 0007505687     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03222.x     Document Type: Article

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