Thin shell morphology in the circumstellar medium of massive binaries

Astronomy and Astrophysics

Volumn 527, Issue 1, 2011, Pages

  Van Marle, A J ^a   Keppens, R ^a,b,c   Meliani, Z ^a  

^a CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

^b FOM INSTITUTE FOR PLASMA PHYSICS RIJNHUIZEN   (Netherlands)

^c UTRECHT UNIVERSITY   (Netherlands)

Author keywords

binaries: general; circumstellar matter; hydrodynamics; stars: massive; stars: winds, outflows

Indexed keywords

3D GRID; ADAPTIVE MESHES; BINARIES: GENERAL; BINARY COMPONENTS; BINARY SYSTEMS; CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; LUMINOUS BLUE VARIABLES; NON-LINEAR; ORBITAL MOTIONS; PARAMETRIC STUDY; PRESSURE BALANCE; RADIATIVE COOLING; STAR SYSTEMS; STAR WINDS; STARS: MASSIVE; STARS: WINDS, OUTFLOWS; STELLAR WIND; THIN SHELLS; WIND VELOCITIES; WOLF-RAYET STARS;

FLUID DYNAMICS; HYDRODYNAMICS; MORPHOLOGY; SHELLS (STRUCTURES); SYSTEMS (METALLURGICAL); THREE DIMENSIONAL; WIND;

STARS;

EID: 78751541340     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015517     Document Type: Article

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