A comprehensive set of simulations of high-velocity collisions between main-sequence stars

Monthly Notices of the Royal Astronomical Society

Volumn 358, Issue 4, 2005, Pages 1133-1158

  Freitag, Marc ^a,b,d   Benz, Willy ^c  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^c UNIVERSITY OF BERN   (Switzerland)

^d NORTHWESTERN UNIVERSITY   (United States)

Author keywords

Galaxies: nuclei; Galaxies: star clusters; Galaxy: centre; Hydrodynamics; Methods: numerical; Stars: interiors

Indexed keywords

ENERGY DISSIPATION; GALAXIES; NUMERICAL METHODS; STARS; VELOCITY;

GALAXIES: STAR CLUSTERS; GALAXIES:NUCLEI; GALAXY CENTER; HIGH VELOCITY COLLISIONS; MAIN SEQUENCE STARS; METHOD: NUMERICAL; RELATIVE VELOCITY; STARS: BE; STARS: INTERIORS; STELLAR STRUCTURE;

HYDRODYNAMICS;

EID: 17744381194     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08770.x     Document Type: Article

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