A comparison of hydrodynamic techniques for modelling collisions between main-sequence stars

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 3, 2007, Pages 997-1005

  Trac, Hy ^a   Sills, Alison ^b   Pen, Ue Li ^c  

^a PRINCETON UNIVERSITY   (United States)

^b MCMASTER UNIVERSITY   (Canada)

^c UNIVERSITY OF TORONTO   (Canada)

Author keywords

Blue stragglers; Globular clusters: general; Hydrodynamics; Methods: numerical; Stars: evolution; Stellar dynamics

Indexed keywords

HYDROGEN; MIXING; NUMERICAL METHODS; STARS;

BLUE STRAGGLERS; EULERIAN; GLOBULAR CLUSTERS:GENERAL; LAGRANGIAN; MAIN SEQUENCE STARS; METHOD: NUMERICAL; SMOOTHED PARTICLE HYDRODYNAMICS; STAR: EVOLUTION; STELLAR DYNAMICS; TOTAL VARIATION DIMINISHING;

HYDRODYNAMICS;

EID: 34248217601     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11709.x     Document Type: Article

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