Line formation in solar granulation VII. CO lines and the solar C and O isotopic abundances

Astronomy and Astrophysics

Volumn 456, Issue 2, 2006, Pages 675-688

  Scott, P C ^a   Asplund, M ^a   Grevesse, N ^b   Sauval, A J ^c  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c ROYAL OBSERVATORY OF BELGIUM   (Belgium)

Author keywords

Convection; Line: profiles; Solar system: formation; Sun: abundances; Sun: infrared; Sun: photosphere

Indexed keywords

COMPUTER SIMULATION; HEAT CONVECTION; HYDRODYNAMICS; INFRARED RADIATION; SOLAR RADIATION; SOLAR SYSTEM;

LINE: PROFILES; SOLAR SYSTEM: FORMATION; SUN: ABUNDANCES; SUN: INFRARED; SUN: PHOTOSPHERE;

ASTROPHYSICS;

EID: 33748759313     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064986     Document Type: Article

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