Radiative hydrodynamics simulations of red supergiant stars

Astronomy and Astrophysics

Volumn 506, Issue 3, 2009, Pages 1351-1365

  Chiavassa, A ^a,b   Plez, B ^b,d   Josselin, E ^b   Freytag, B ^c,d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIV MONTPELLIER   (France)

^c UNIVERSITÉ DE LYON   (France)

^d UPPSALA UNIVERSITY   (Sweden)

Author keywords

Hydrodynamics; Radiative transfer; Stars: atmospheres; Stars: supergiants; Techniques: interferometric

Indexed keywords

3D SIMULATIONS; CLOSURE PHASIS; CONVECTIVE CELL; HYDRODYNAMICS SIMULATIONS; INTENSITY DISTRIBUTION; INTENSITY MAPS; MASS-LOSS; POSITION ANGLE; RADIATIVE TRANSFER CODES; STARS: ATMOSPHERES; STARS: SUPERGIANTS; SURFACE INHOMOGENEITIES; TECHNIQUES: INTERFEROMETRIC;

FLUID DYNAMICS; GRANULATION; HYDRODYNAMICS; INTERFEROMETRY; RADIATIVE TRANSFER; THREE DIMENSIONAL; THREE DIMENSIONAL COMPUTER GRAPHICS; VISIBILITY;

STARS;

EID: 70350747583     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911780     Document Type: Article

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