Granulation in K-type dwarf stars: II. Hydrodynamic simulations and 3D spectrum synthesis

Astronomy and Astrophysics

Volumn 501, Issue 3, 2009, Pages 1087-1101

  Ramirez I ^a,b   Allende Prieto, C ^b,c   Koesterke, L ^d   Lambert, D L ^b   Asplund, M ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b The University of Texas at Austin   (United States)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

^d UNIVERSITY OF TEXAS AT AUSTIN   (United States)

Author keywords

Stars: atmospheres; Stars: late type; Sun: granulation

Indexed keywords

3D MODELS; CHEMICAL COMPOSITIONS; DWARF STARS; EQUIVALENT WIDTH; FUNDAMENTAL CHARACTERISTICS; HYDRODYNAMIC SIMULATION; LINE PROFILES; LINE STRENGTH; MODEL ATMOSPHERE; MODEL PREDICTION; NON-LTE; REFERENCE STAR; SPECTRUM SYNTHESIS; STARS: ATMOSPHERE; STARS: LATE-TYPE; STELLAR ROTATION; STELLAR SPECTRA; SUN: GRANULATION; SURFACE INHOMOGENEITIES; THEORETICAL VALUES; WAVELENGTH SHIFT;

FORECASTING; GRANULATION; HYDRODYNAMICS; STARS; THREE DIMENSIONAL COMPUTER GRAPHICS; WAVELENGTH;

THREE DIMENSIONAL;

EID: 76949103684     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911741     Document Type: Article

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