A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type stars

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Mashonkina, L ^a,b   Gehren, T ^a   Shi, J R ^c   Korn, A J ^d   Grupp, F ^a,e  

^a UNIVERSITY OF MUNICH   (Germany)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d UPPSALA UNIVERSITY   (Sweden)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

atomic data; atomic processes; line: formation; stars: atmospheres; stars: fundamental parameters

Indexed keywords

ATOMIC DATA; ATOMIC PROCESS; LINE: FORMATION; STARS: ATMOSPHERES; STARS: FUNDAMENTAL PARAMETERS;

ATOMIC SPECTROSCOPY; ATOMS; HYDROGEN; IONIZATION; SOLAR POWER GENERATION;

STARS;

EID: 79952322475     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015336     Document Type: Article

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