3D LTE spectral line formation with scattering in red giant stars

Astronomy and Astrophysics

Volumn 529, Issue , 2011, Pages

  Hayek, W ^a,b,c   Asplund, M ^a   Collet, R ^a   Nordlund, A ^d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^c UNIVERSITY OF EXETER   (United Kingdom)

^d UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Line: formation; Radiative transfer; Stars: atmospheres

Indexed keywords

FLUID DYNAMICS; GIANT STARS; GRANULATION; HYDRAULICS; IRON COMPOUNDS; OPACITY; PHOTOIONIZATION; PHOTONS; RADIATIVE TRANSFER; SPECTROSCOPY; TEXTURES; VELOCITY;

CONTINUUM SCATTERING; EXCITATION POTENTIALS; ISOTROPIC SCATTERING; LINE: FORMATION; LOCAL THERMODYNAMIC EQUILIBRIUM; SPECTRAL LINE PROFILES; STARS: ATMOSPHERE; STELLAR ATMOSPHERES;

COHERENT SCATTERING;

EID: 79955385083     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015782     Document Type: Article

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