Thorium-rich halo star HD 221170: Further evidence against the universality of the r-process

Astronomy and Astrophysics

Volumn 430, Issue 1, 2005, Pages 255-262

  Yushchenko, A ^a,b   Gopka, V ^b   Goriely, S ^c   Musaev, F ^d,e,f   Shavrina, A ^e   Kim, C ^g   Woon Kang, Y ^a   Kuznietsova, J ^e   Yushchenko, V ^b  

^a Sejong University   (South Korea)

^b ODESSA NATIONAL UNIVERSITY   (Ukraine)

^c UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^d RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^e INSTITUTE OF HYDROBIOLOGY   (Ukraine)

^f Shamakhy Astrophysical Observatory Azerbaijan   (Azerbaijan)

^g Chonbuk National University   (South Korea)

Author keywords

Line: identification; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: atmospheres; Stars: evolution; Stars: individual: HD 221170

Indexed keywords

ASTROPHYSICS; COMPOSITION; IRON; OPTICAL RESOLVING POWER; SIGNAL TO NOISE RATIO; TELESCOPES;

ABUNDANCES; LINE: IDENTIFICATION; NUCLEAR REACTIONS; NUCLEOSYNTHESIS; STARS: ABUNDANCES; STARS: ATMOSPHERES; STARS: EVOLUTION; STARS: INDIVIDUAL: HD 221170;

THORIUM;

EID: 12844260188     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041540     Document Type: Article

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