Non-LTE calculations for neutral Na in late-type stars using improved atomic data

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Lind, K ^a,b   Asplund, M ^b   Barklem, P S ^c   Belyaev, A K ^d  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UPPSALA UNIVERSITY   (Sweden)

^d HERZEN STATE PEDAGOGICAL UNIVERSITY OF RUSSIA   (Russian Federation)

Author keywords

line: formation; stars: abundances; stars: late type

Indexed keywords

ATOMIC DATA; CHARGE EXCHANGE REACTIONS; COLLISIONAL EXCITATION; IMPACT EXCITATION; IONISATION; LATE-TYPE STARS; LINE STRENGTH; LINE: FORMATION; LOCAL THERMODYNAMIC EQUILIBRIUM; NEUTRAL HYDROGEN; NON-LTE; QUANTUM-MECHANICAL CALCULATION; STARS: ABUNDANCES; STARS: LATE-TYPE; STATISTICAL EQUILIBRIUM; STELLAR ATMOSPHERES; STELLAR PARAMETERS; WEAK LINES;

CHARGE TRANSFER; HYDROGEN; ION EXCHANGE; QUANTUM THEORY; SODIUM;

STARS;

EID: 79952433180     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016095     Document Type: Article

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