Line formation in solar granulation VI. [Cl], Cl, CH and C2 lines and the photospheric C abundance

Astronomy and Astrophysics

Volumn 431, Issue 2, 2005, Pages 693-705

  Asplund, M ^a   Grevesse, N ^b   Sauval, A J ^c   Allende Prieto, C ^d   Blomme, R ^c  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c ROYAL OBSERVATORY OF BELGIUM   (Belgium)

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

Author keywords

Convection; Line: formation; Stars: atmospheres; Sun: abundances; Sun: granulation; Sun: photosphere

Indexed keywords

ASTROPHYSICS; ERROR ANALYSIS; GRANULATION; HYDRODYNAMICS; MOLECULAR DYNAMICS; PROBABILITY; SENSITIVITY ANALYSIS; VIBRATION MEASUREMENT;

CONVECTION - LINE: FORMATION; STARS: ATMOSPHERES; SUN: ABUNDANCES; SUN: GRANULATION; SUN: PHOTOSPHERE;

SOLAR SYSTEM;

EID: 13944268868     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041951     Document Type: Article

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