The chemical composition of the mild barium star HD 202109

Astronomy and Astrophysics

Volumn 413, Issue 3, 2004, Pages 1105-1114

  Yushchenko, A V ^a   Gopka, V F ^a,e   Kim, C ^b   Liang, Y C ^g,h,i   Musaev, F A ^c,d,e,f   Galazutdinov, G A ^c,e,f  

^a ODESSA NATIONAL UNIVERSITY   (Ukraine)

^b Chonbuk National University   (South Korea)

^c INSTITUTE OF HYDROBIOLOGY   (Ukraine)

^d RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^e ISAAC NEWTON INSTITUTE OF CHILE   (Chile)

^f SAO Branch   (Russian Federation)

^g CHINESE ACADEMY OF SCIENCES   (China)

^h UNIVERSITÉ PARIS DIDEROT   (France)

ⁱ UNIVERSITY OF MUNICH   (Germany)

Author keywords

Line: identification; Stars: abundances; Stars: atmospheres; Stars: binaries; Stars: evolution; Stars: individual: HD 202109

Indexed keywords

ATMOSPHERIC TURBULENCE; BARIUM; COMPOSITION; DATA REDUCTION; NEUTRONS; SIGNAL TO NOISE RATIO; SOLAR SYSTEM; SPACE RESEARCH; SPECTROMETRY; SPECTRUM ANALYSIS;

MICROTURBULENCE; NUCLEOSYNTHESIS; STARS;

ASTRONOMY;

EID: 0742286187     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031596     Document Type: Article

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