Three-dimensional hydrodynamical simulations of red giant stars: Semi-global models for interpreting interferometric observations

Astronomy and Astrophysics

Volumn 524, Issue 4, 2010, Pages

  Chiavassa, A ^a   Collet, R ^a   Casagrande, L ^a   Asplund, M ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

hydrodynamics; radiative transfer; stars: atmospheres; stars: horizontal branch; stars: individual: HD 214868; techniques: interferometric

Indexed keywords

ASTROPHYSICS; BEHAVIORAL RESEARCH; FLUID DYNAMICS; GRANULATION; HEAT CONVECTION; HYDRODYNAMICS; INTERFEROMETERS; INTERFEROMETRY; RADIATIVE TRANSFER; THREE DIMENSIONAL; THREE DIMENSIONAL COMPUTER GRAPHICS;

3D MODELS; 3D SIMULATIONS; CLOSURE PHASE; EFFECTIVE TEMPERATURE; GALACTIC CHEMICAL EVOLUTIONS; INTENSITY MAPS; K BANDS; LIMB DARKENING; METALLICITIES; POSITION ANGLE; RADIATIVE TRANSFER CODES; RED GIANT BRANCHES; RED GIANTS; SEMI-GLOBAL; SHORTER WAVELENGTH; SPATIAL FREQUENCY; STARS: ATMOSPHERES; STARS: HORIZONTAL-BRANCH; STARS: INDIVIDUAL: HD 214868; STELLAR DISKS; SURFACE CONVECTION; SURFACE GRAVITY; TECHNIQUES: INTERFEROMETRIC; THEORETICAL PREDICTION; ZERO POINT;

STARS;

EID: 78649505630     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015507     Document Type: Article

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