Dynamical friction for dark halo satellites: Effects of tidal mass loss and growing host potential

Monthly Notices of the Royal Astronomical Society

Volumn 351, Issue 3, 2004, Pages 891-902

  Zhao, HongSheng ^a,b,c  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c Beijing Observatory   (China)

Author keywords

Galaxies: dwarf dark matter; Galaxy: halo; Galaxy: kinematics and dynamics; Methods: analytical

Indexed keywords

ANALYTICAL MODELS; ASTROPHYSICS; BLACK HOLES; DECAY (ORGANIC); GRAVITATION; ORBITS; PLANETS; SATELLITES; STARS; TRIBOLOGY;

DARK MATTER; DYNAMICAL FRICTIONS; GALAXIES: DWARF; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY: DWARF-DARK MATTER; GALAXY:HALO; HOST GALAXIES; MASS LOSS; METHODS:ANALYTICAL; ORBITAL DECAY;

FRICTION;

EID: 3042814730     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07835.x     Document Type: Article

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